{"as_of":"2026-08-16T05:40:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0d0fead45717732abb8519d930e90ce8863edfd89bcc662d7f3151084ed503e7","coverage":[{"denominator":104,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:25:44.363520Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/1908.09198/citation-record","integrity":"/paper/1908.09198/integrity","json":"/paper/1908.09198/citation-record.json","paper":"/paper/1908.09198"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.005128Z","title":"1947, Monthly Notices of the Royal Astronomical Society, 107, 211","venue":null,"work_id":null,"year":1947},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.005128Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:610b45020b8eca23e13ef16a9a20819976b481f908608d9d222f7889da80a70a","observation_id":"62e72b66-fc80-4f99-a062-8a77e5bd114d","resolution":{"observed_at":"2026-08-14T11:25:44.005128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.009304Z","title":"2019, The Astrophysical Journal Supplement Series, 243, 20","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.009304Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:92c609447126324fe8e1bc810e472caf575773fb9e2b76a1e357736c82db4089","observation_id":"9417d0bb-a004-4696-91d4-041e2eb5a9af","resolution":{"observed_at":"2026-08-14T11:25:44.009304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.013071Z","title":"W., & Cox, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.013071Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d98e59fa73bf019208892d5714b9ffd8133b518a1a0b70f80012acadbcb72e7e","observation_id":"c60f2a87-6903-46fe-bdb4-785911f9d006","resolution":{"observed_at":"2026-08-14T11:25:44.013071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.016934Z","title":"1986, Physical review letters, 57, 2807","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.016934Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:7c86dd78eaf40a86543d1325788f5f040c08957bdfd9379874268673b2c79aca","observation_id":"c7efde08-4d17-46f6-8be2-bc33a4424d8d","resolution":{"observed_at":"2026-08-14T11:25:44.016934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.020832Z","title":"2009, Physical review letters, 103, 211101","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.020832Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:2578d71177be7ab036d0dc9e348095994f6c45745ec894ed40dce07e90a771fc","observation_id":"848b95e9-201f-47b7-bf10-df0d45cd2976","resolution":{"observed_at":"2026-08-14T11:25:44.020832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.024904Z","title":"1993, Geophysical research letters, 20, 2323","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.024904Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:86fb9ec3f5380c42a6e53556b5287bce68a096da6f37393ae7cb9b47b0ed0f2d","observation_id":"831d5c67-3b09-4d25-b556-7267228cd885","resolution":{"observed_at":"2026-08-14T11:25:44.024904Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.029330Z","title":"2009, Physics of Plasmas, 16, 052106","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.029330Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:64bd42a8930919aaccc2d9aa1cb654231c360b6876f79414362ec2a57ed6171a","observation_id":"1c3440a7-0ee7-4d7f-856a-9a7a9b0fc532","resolution":{"observed_at":"2026-08-14T11:25:44.029330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.032986Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.032986Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d32b64846db98265d6776e6bcf48566b5ac8da018117801c3bd7ede3af4dc7d4","observation_id":"a5bfa9a3-e707-448b-81bd-13291db2e27c","resolution":{"observed_at":"2026-08-14T11:25:44.032986Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.036565Z","title":"E., & Funsten, H","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.036565Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:c6e79008c04b6e6f0d8e23673de0d4044367fb8bd98d7d851da1ec8eed0fe759","observation_id":"9863def5-af63-42e4-9e9e-31e2185f3eb5","resolution":{"observed_at":"2026-08-14T11:25:44.036565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.039993Z","title":"2005, Living Reviews in Solar Physics, 2, 4","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.039993Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:2246503fc638cd5b4a0a1c9df1e75378ca221a1876f8fd7a4d5ac65c74c8e49d","observation_id":"b966f335-460d-4006-9efa-d0f36207bc6f","resolution":{"observed_at":"2026-08-14T11:25:44.039993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.043556Z","title":"A., & Mace, R","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.043556Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:4df6d825006125c569d83875f5bf8afac8b3486c8e5b3d28c1e8cc51bd33fa5e","observation_id":"831e575c-d2f3-4c77-949b-2095a02533f2","resolution":{"observed_at":"2026-08-14T11:25:44.043556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.047085Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.047085Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:70ccfc724bd09d61a14e35f5482352acaf05a8cca452bf0a18c642efd36c8654","observation_id":"c1ec42ff-687e-49fc-ba24-2f037893069b","resolution":{"observed_at":"2026-08-14T11:25:44.047085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.050639Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.050639Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:7f93d5300bbc35aaa9d73ec47fdc526ecb64efac100ba0cada1af27f60ddcf4f","observation_id":"0544fe30-08ff-459d-a9d6-50ddb9e75ebe","resolution":{"observed_at":"2026-08-14T11:25:44.050639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.054049Z","title":"1929, MNRAS, 89, 456","venue":null,"work_id":null,"year":1929},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.054049Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:0275b88fde81226bab34cab2237a7569a4d871f088d814cdb3f2ad75b0dc0d3f","observation_id":"84356e77-0146-40bd-be54-5aba248097f6","resolution":{"observed_at":"2026-08-14T11:25:44.054049Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.057566Z","title":"R., Moore, T","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.057566Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:5d56b924b8a34f26c9415b141ba64136aee436e48dbba5e8b1455534bb2e33df","observation_id":"3b5d62a8-9f2f-4953-8184-cffd1c260684","resolution":{"observed_at":"2026-08-14T11:25:44.057566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.061022Z","title":"2010, Physical review letters, 104, 255002","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.061022Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:973431bcdb5dc06a8a68cc46242d99ac3502477c519800ce39c42b4ad840f664","observation_id":"a6f84ba8-bc8d-4abf-97af-a21b1f3bbd9d","resolution":{"observed_at":"2026-08-14T11:25:44.061022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.064347Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.064347Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:5dc97a6ab1ae128caf83293cd26935fb49c55d90eacecf2bbc67044ef90fd190","observation_id":"fc469fea-69c7-43d9-b63b-7487ae23acb0","resolution":{"observed_at":"2026-08-14T11:25:44.064347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.067928Z","title":null,"venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.067928Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:a2162c17cfb09f5847cde51fd8b9990ee08bd2449bb63aa91b32a95a930ca4ff","observation_id":"dddfcab2-c2a6-4826-a67b-859f3b18131f","resolution":{"observed_at":"2026-08-14T11:25:44.067928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.071167Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.071167Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:707d813176933f04f41f917bbc68c5471d57232be049b8e5e3893031ec8e1657","observation_id":"81f43873-54bd-44d8-9add-13f95ed0666a","resolution":{"observed_at":"2026-08-14T11:25:44.071167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.074579Z","title":"R., Gibson, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.074579Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:ed12d0f61e3607f65d9687d967db742ace088fc06a17cd2e8c008d3e734611a5","observation_id":"febbecc5-801e-468d-9eaf-c8382a36dbd7","resolution":{"observed_at":"2026-08-14T11:25:44.074579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.078244Z","title":"1990, Planetary and Space Science, 38, 1091","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.078244Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d49752fed3ef526d3bd8fc5af4ac2c97d24d746a74345fd54afee6ca85199dc7","observation_id":"715f7c73-9130-4243-a499-98c4b0a9c4ea","resolution":{"observed_at":"2026-08-14T11:25:44.078244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.081401Z","title":"G., & Schunk, R","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.081401Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:3dc8c8d45aee3cb05de21ea3efe5ee2016e89c2ceccf3d86a40e469605864ef4","observation_id":"818be998-4850-40d7-8c45-4de9d6f40c31","resolution":{"observed_at":"2026-08-14T11:25:44.081401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.084624Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.084624Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:a371d44c213e43e6e0c7962ef1dea340dcdeba50e1915a29dbc8aa6f76a6e59f","observation_id":"6684dda1-7882-431a-95e8-e674c3d92845","resolution":{"observed_at":"2026-08-14T11:25:44.084624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.088442Z","title":"1971, ApJ, 166, 669","venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.088442Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:822cfef10ec2318dcd039288c324cbbea6c2aee57135e7580c90b3a0698259c5","observation_id":"7c4e3f24-7431-45b4-b3ae-c8e787c6c1b0","resolution":{"observed_at":"2026-08-14T11:25:44.088442Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.243417Z","title":"R., & Roberts, P","venue":null,"work_id":"a0af66b5-2f41-4e34-a308-cd15e59c49be","year":1971},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.091997Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:0336e9c842c85dffd54973e9b2eba189da26b7f0db118ad5849178b2ed32235a","observation_id":"ad1dd259-a1f9-40df-801b-1a1c77d4a898","resolution":{"observed_at":"2026-08-14T11:25:45.247008Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.232405Z","title":null,"venue":null,"work_id":"c6c97142-b054-42ae-a70f-386baa940699","year":1964},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.095527Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:9441cdb8742448a9ea6b95a980c3ff770dd73ac7d26a4a855922d8a967c0e5a0","observation_id":"408e4968-f7b1-4a2f-bda1-bd26c04bd4a9","resolution":{"observed_at":"2026-08-14T11:25:45.236250Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.221701Z","title":"2016, Journal of Geophysical Research (Space Physics), 121, 9340","venue":null,"work_id":"6c3e12ce-2f27-498b-91b9-05066b7c5a4f","year":2016},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.098964Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:44a9ee56ff3cdacec3abd188616ecf8a679f884f4ede02021763db11a8bc4264","observation_id":"f2cea405-23ae-43b5-bb97-c13a047a78a4","resolution":{"observed_at":"2026-08-14T11:25:45.225471Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.102535Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.102535Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:4bee3aa3dd9c5ada1542b289aaf58c7d6ac4d26751872aeb87abc1e36bb74db7","observation_id":"86c7be4c-cbe0-45ab-ab2c-79991d8aed2d","resolution":{"observed_at":"2026-08-14T11:25:44.102535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.204137Z","title":null,"venue":null,"work_id":"8e0b65aa-bc98-45ef-b943-df0c6d2c6eb2","year":2005},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.106578Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:f9b134acfd94b9caee1a666b7a23d6796c0846e3f9696c1a0fd6038f6aa7e056","observation_id":"e89fb7ef-80d0-41d1-bf2b-e2a99beb2567","resolution":{"observed_at":"2026-08-14T11:25:45.207932Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.193349Z","title":"D., & Gary, S","venue":null,"work_id":"bfa52aec-9b9c-4ebf-a3bd-1c2f1192429c","year":1975},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.110366Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:f08166830eabc5d92ee5d5359271692252dafc03afb96b51387f85ec3308b5e9","observation_id":"e5dd0d46-d702-4c87-89c0-8f55eb6731a1","resolution":{"observed_at":"2026-08-14T11:25:45.197229Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.182773Z","title":null,"venue":null,"work_id":"2d3bc282-86b4-4a03-b7fe-d5972da39fbb","year":1971},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.114007Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:1273cb3de9049608e30ba8ce5bcb4d573fe6d08d29da0dc4b3f822b934a92a45","observation_id":"49bcc798-92b0-4bb4-901f-40f571a1c7dd","resolution":{"observed_at":"2026-08-14T11:25:45.186310Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.171426Z","title":"P., & Karimabadi, H","venue":null,"work_id":"65d332ec-e6e3-437d-affc-fa0769398df9","year":2006},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.117699Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:e3ae09c01b7c88e588b5ab5e30f5b763d80d08f5e130fae3003a8d1f33156c61","observation_id":"38833c30-fb2f-47f6-8ba6-e36a9442a3b7","resolution":{"observed_at":"2026-08-14T11:25:45.175434Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.160454Z","title":"P., & Wang, J","venue":null,"work_id":"b23f7bf8-90c0-4eeb-80f9-68319c53253f","year":1996},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.121316Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:05134efff9464ee146f755164070713b693b1046375e8dcb56a8dcd01a80e144","observation_id":"d66369d4-9f01-454b-a765-36a54026fd9b","resolution":{"observed_at":"2026-08-14T11:25:45.164024Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.150031Z","title":"1995, SSRv, 72, 49","venue":null,"work_id":"785ac570-da7a-4424-a8d4-c5b4b3b40b70","year":1995},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.124652Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:ad2f1429cdd77022baa503d8faeb11f33b205e4825eaf9bbffba5507b68a8d27","observation_id":"ac433c65-d8f8-430a-b67b-15fc38f1d4b6","resolution":{"observed_at":"2026-08-14T11:25:45.153668Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.139393Z","title":"J., Adolfo, F., Dorelli, J","venue":null,"work_id":"d0f77ca4-4272-4a9b-a706-404120890c7c","year":2017},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.128169Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:4eb02aa5c518e4ab940e82b7228a5b52fe1ba5e07bc88f0a36b277aed97b855e","observation_id":"629daed7-119d-4a41-810f-a5657676734b","resolution":{"observed_at":"2026-08-14T11:25:45.142856Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.128151Z","title":null,"venue":null,"work_id":"63183a9f-60d1-4ed2-ade5-527e808304ac","year":2018},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.131631Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:514834b666a4a66f1fdb60dda58b8b7e806121b78784ce41fd73254f3fe52b0d","observation_id":"96cf1c9b-504a-4c6f-87a1-916df4a38374","resolution":{"observed_at":"2026-08-14T11:25:45.131826Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.116605Z","title":"H., Goedbloed, J., & Poedts, S","venue":null,"work_id":"b73bcf0e-1149-4d75-8c76-bb5b41d8c7c8","year":2004},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.136398Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:1eaa3c6e33bce46892495d6349128bfcba41e9ae7cb4f494eef27ab2301b3b39","observation_id":"b31ede84-24fb-4c99-aff2-65bacd963bcd","resolution":{"observed_at":"2026-08-14T11:25:45.120595Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.139897Z","title":"1995, ApJ, 438, 763","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.139897Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:30b158ad86e4c43345ec007767623a9858b1b948750f3fff03b4d06c51bfdf34","observation_id":"4575b0c2-f050-4bd1-881d-bef76a45b811","resolution":{"observed_at":"2026-08-14T11:25:44.139897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.097846Z","title":null,"venue":null,"work_id":"310ffe38-ac81-4850-b730-705b0aa4e41d","year":1991},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.143590Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:8490c5d1c755a49a0503c376a5e2c6d876eeb3cdb960fc28b6dac019e4fddb5b","observation_id":"bd075a87-77b8-49b2-bd90-5b32fab3c958","resolution":{"observed_at":"2026-08-14T11:25:45.101744Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.087594Z","title":"J., Beer, J., Geller, M., et al","venue":null,"work_id":"bff41661-9757-4bee-957c-086b71d77bd9","year":2010},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.147240Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:ee6ab5dbf58e429d3b4895ce330cb8f4a83342876839b2b43fca3d9a36fd966d","observation_id":"37876179-4692-45b1-a853-3029c11b67a6","resolution":{"observed_at":"2026-08-14T11:25:45.090955Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.076858Z","title":"E., & Sturrock, P","venue":null,"work_id":"017988c1-ac45-4076-9ff5-bfb64f0edf72","year":1968},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.150819Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:a6a223623e0d2382f2641dc9336c8fdd3a784f8c8b41cbb2c605252b5929a959","observation_id":"22713c2b-4430-43bf-ba42-a49af7941dc2","resolution":{"observed_at":"2026-08-14T11:25:45.080967Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.066690Z","title":null,"venue":null,"work_id":"fb272394-43b4-438e-afec-eb583b38bd00","year":2006},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.155077Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:f29f258974b7ed1b9f50b79c09f54b1db1be722fe76d3a4b1e9e0f0c9251db61","observation_id":"a65d1f93-aa08-4ef8-babe-5b3b6e940d9a","resolution":{"observed_at":"2026-08-14T11:25:45.070105Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.055967Z","title":null,"venue":null,"work_id":"ac79311b-017f-46dd-81d9-00d284db751f","year":1981},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.159527Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:09eab6d5b4a265ba0363deb86ab1e2b977a40785d69da6cf194d78b8c30f10d1","observation_id":"538f9b79-5d65-46ff-97a8-1758c520ad27","resolution":{"observed_at":"2026-08-14T11:25:45.059607Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.044876Z","title":null,"venue":null,"work_id":"c6326c69-d108-46db-8359-4c022116d84f","year":2008},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.163142Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:6c5e0e4eb37a6a49815bfcb38e61eda494fe37741e87d97073c65dadb2c6b262","observation_id":"b8144f5d-fd57-4af0-a666-824ecf4785d7","resolution":{"observed_at":"2026-08-14T11:25:45.048589Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.033756Z","title":"G., TenBarge, J","venue":null,"work_id":"90cd6f5d-5b4b-413d-8efe-d311702ec6d3","year":2011},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.166753Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:13c86a964b4159e38dcc3a77e69fafe8c1dc0568d2dde16ecb76b8f70a34df4e","observation_id":"be2bd4df-b790-4654-b4e9-5ccb2024ae2a","resolution":{"observed_at":"2026-08-14T11:25:45.037532Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.021503Z","title":"Q., Esser, R., & Habbal, S","venue":null,"work_id":"2d38f4b9-8d76-4a55-946d-037ed48e2b28","year":1997},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.170995Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d798a30f1417c578a7abc9d146d3edc0febf2b10b1ed5ac4c7996889be76865f","observation_id":"71435a47-cc11-496e-803b-8cff7abe6d5f","resolution":{"observed_at":"2026-08-14T11:25:45.025893Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:45.009441Z","title":"W., Liu, S., & Petrosian, V","venue":null,"work_id":"3d1d4923-27a4-405e-a86b-4028f5269a66","year":2009},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.174497Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:b99e6db00b3e036ec5fb5c151b57b1d94cb0aafccc52af0e2d1bd17f92e0333b","observation_id":"d4e3f30c-dfa8-4892-9adb-dfd94ad8250c","resolution":{"observed_at":"2026-08-14T11:25:45.013448Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.997323Z","title":"1968, The Physics of Fluids, 11, 1797","venue":null,"work_id":"8c29002a-e356-4850-885d-25fa1bdb5946","year":1968},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.178370Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d7c2d4a90afe03df056ac6c6401886e74f2b99b77234863c1a4dcbe70f8723ff","observation_id":"52982fc0-c3b1-47db-b64d-61cffa8d0040","resolution":{"observed_at":"2026-08-14T11:25:45.001798Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.985801Z","title":"C., Lazarus, A","venue":null,"work_id":"367c8f9f-fa1e-4b2b-be61-86cbdb5d9b03","year":2002},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.181879Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:ec926ae40a3c54b9c5a488a093e683c8f29f043ded979a81e9622fcaa9e594b6","observation_id":"cd1d7e52-8c8a-4f94-9126-2ec4b441efee","resolution":{"observed_at":"2026-08-14T11:25:44.989886Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.974794Z","title":"W., & Szabo, A","venue":null,"work_id":"13dc10fa-4efe-4b55-a70f-44695e33ceff","year":2006},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.185732Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d1aa41a29412d7e9bf72c9f1a2d75acb640828830c67e6d26633d5745ac071fa","observation_id":"841e7ecf-cadc-4b40-9ec1-19bd48d3baa5","resolution":{"observed_at":"2026-08-14T11:25:44.978655Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.964149Z","title":"A., & Holzer, T","venue":null,"work_id":"9ebf524d-ba31-48c0-9955-f9e18e6eb34c","year":1976},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.189147Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:cff62cba9a9ad63e91a39e38a7456d3c13fb8ea4d57ea4204966133d81d01191","observation_id":"360eef1b-9a16-477f-be62-ef6f85b6d69a","resolution":{"observed_at":"2026-08-14T11:25:44.967648Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.192712Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.192712Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:2bd9bb8b634f9f14ad415c1935b19bb1413067d6e9b3bb7f4625813296462229","observation_id":"189edaf5-5411-4e83-8697-6a1f8f447fcf","resolution":{"observed_at":"2026-08-14T11:25:44.192712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.946978Z","title":"2008, ApJ, 685, 1270 Le Chat, G., Issautier, K., & Meyer-Vernet, N","venue":null,"work_id":"1988075d-6e76-4d4a-be43-170c87e7c0fc","year":2008},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.196399Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:7b653627be2a30ca47c7098de2083f3ef152d86387d3e1bd249862c6b7c3c9f9","observation_id":"6282bc80-05ff-4546-aca7-bb305cd25e7f","resolution":{"observed_at":"2026-08-14T11:25:44.950754Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.935512Z","title":"2006, PhRvD, 73, 044001 Lie-Svendsen, Ø., Leer, E., & Hansteen, V","venue":null,"work_id":"a457153b-25ad-4848-bb5c-791604b194b3","year":2006},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.200065Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:40fd2fbebd69dd04b10b5af9fde8c82048e9fa17ba9e8e5143718cdf272610ce","observation_id":"092b4418-e972-48bf-aba8-7f2ab5bf78a2","resolution":{"observed_at":"2026-08-14T11:25:44.939645Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.924596Z","title":null,"venue":null,"work_id":"61d6e49f-8bef-4e8f-a360-ad987760007a","year":1980},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.203501Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d62ab239299a75681bb6b0472e66922c334ac7fa8dab47353731f9ee8b29151b","observation_id":"77bad4f0-555f-46d0-ab9a-9e744725f59e","resolution":{"observed_at":"2026-08-14T11:25:44.927892Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.914176Z","title":"2017, Kappa distributions: theory and applications in plasmas (Elsevier)","venue":null,"work_id":"7d56664a-cb25-4471-8d07-139d1f1be7eb","year":2017},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.207322Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:b1f5ca797f948eb261d93c6dde87ff2909f50dd050abcafc98fa00da7a808455","observation_id":"72a29ba6-7ad7-4e91-be72-3c2fc8b1bcd1","resolution":{"observed_at":"2026-08-14T11:25:44.917925Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.211007Z","title":"2013, Space Science Reviews, 175, 183","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.211007Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:7a00c3e76fee7a27e2ed41d5821446c0bb32ae5ba322927e529eac4653ffdfb5","observation_id":"5d30b954-0a21-4e08-b3c3-d7e32e1f5e0c","resolution":{"observed_at":"2026-08-14T11:25:44.211007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.897276Z","title":"L., & Lotko, W","venue":null,"work_id":"54d68565-ace0-4eb0-8e76-d16ac48f9a92","year":1996},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.214393Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:96cbae03495ff9ed92cdd0f470e67f6d31daa1af3324b22440e0774a2e807ece","observation_id":"639ca2f4-b621-474d-9110-0fd45ea8eba6","resolution":{"observed_at":"2026-08-14T11:25:44.900831Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.886888Z","title":"2001, ApJ, 554, 1175","venue":null,"work_id":"b0a8718b-1efa-4a11-b806-7ebf3d77d86f","year":2001},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.217724Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:730f5c4762dce794029e206f8f07dae335bca031e1c527cb20021371c8f6c9a6","observation_id":"19458984-9e00-45a7-9500-8ca6ba46ead2","resolution":{"observed_at":"2026-08-14T11:25:44.890303Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.221119Z","title":"2006, Living Reviews in Solar Physics, 3, 1","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.221119Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:91a5db063b9fc1832eb473ed38251439e82b6722a7e57008d161077e9df833e5","observation_id":"0650f230-072b-4e74-9831-a930ffed3462","resolution":{"observed_at":"2026-08-14T11:25:44.221119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.868753Z","title":null,"venue":null,"work_id":"ba39f095-3434-4ad8-b190-b9a1af4e8b6c","year":1982},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.224790Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:b7b51c2de5e66b35a8111ee5695f4c58c2dc3f879f2ccf6cf2d36c0707ae24b2","observation_id":"19ffdab2-7a6a-4c1d-bb75-feb603e3f6a9","resolution":{"observed_at":"2026-08-14T11:25:44.872317Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.857790Z","title":"J., Ebert, R","venue":null,"work_id":"d74aeaa0-6a8b-444e-a293-628ea839cc93","year":2008},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.228329Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:b43512ec64686a57cee9fc932634dc21436ea213013a2f9e27f63dfbb91a4561","observation_id":"c3c2edc8-7174-4549-b32d-ae99be3fe060","resolution":{"observed_at":"2026-08-14T11:25:44.861438Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.846116Z","title":"J., Barraclough, B","venue":null,"work_id":"9fc86b08-61f2-4a6a-a47f-ee98fbb18631","year":2000},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.231721Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:8ec2f166bb2d10e2d668e4ca1aee6e76bae015d832d78b0001cd9c869a463ddc","observation_id":"2c618d87-f68e-4e4a-b3bc-0445a08ad245","resolution":{"observed_at":"2026-08-14T11:25:44.849955Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.834955Z","title":"2012, Numerical solution of partial differential equations, Vol","venue":null,"work_id":"e9cfeaab-2648-43fd-90c9-0697f82e254e","year":2012},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.235690Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:ea91949b92085b1be7cdf84a3040939495ceb48461d4c53cc91bb8ca2568e7a1","observation_id":"3cc49883-3c3d-4229-a8f2-3fc360d87ccb","resolution":{"observed_at":"2026-08-14T11:25:44.838836Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.823934Z","title":null,"venue":null,"work_id":"d42bbf42-c359-455c-a40f-49ffec87045f","year":2015},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.239199Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:d5b9692748becd84d1865fa0cd2f9abcde29e5e57df248837618ca1dd562b805","observation_id":"bb535df9-1b44-4e71-9c84-37bf9191fa1c","resolution":{"observed_at":"2026-08-14T11:25:44.827887Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.242871Z","title":"2007, Basics of the solar wind (Cambridge University Press)","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.242871Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:8e44c4d87cd8bdd45b09a6b1eb9389233f45d4aca0f79ca2ecca102b408ffce3","observation_id":"55db18d4-0e2e-4e19-8aa7-ac29aa3c3b5d","resolution":{"observed_at":"2026-08-14T11:25:44.242871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.806131Z","title":"J., Tomczyk, S., & Pinto, R","venue":null,"work_id":"a950363a-159f-4cf1-9be8-89b4537e416d","year":2015},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.246177Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:c8ee217a814ae1be2ed2dae1258e5fda443d12d86da0d9035071d64e00150af6","observation_id":"4b81979d-6669-4f11-a639-50640d3f0923","resolution":{"observed_at":"2026-08-14T11:25:44.810044Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.793976Z","title":"1998, Journal of Geophysical Research: Space Physics, 103, 9553","venue":null,"work_id":"8cf00441-2d32-4d7f-8039-a51f790c2d47","year":1998},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.250009Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:1b88decd9da15203fe7eb135120e7f13a72dc87f4d0a66d64f952f54e39e7858","observation_id":"8f38fbe0-63fa-462d-b961-57b146de07f9","resolution":{"observed_at":"2026-08-14T11:25:44.798596Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.782965Z","title":"1968, in Physics of the Magnetosphere (Springer), 641–659","venue":null,"work_id":"e69ae0cd-de57-4de0-a3b2-9b65cd843ee9","year":1968},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.254393Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:47026d57778e508065a39999dc830203a37946e03a1f68a84bd792dea884169c","observation_id":"dcad92f3-4cc7-4fb6-829a-07d04181e792","resolution":{"observed_at":"2026-08-14T11:25:44.786698Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.772205Z","title":"1958, The Physics of Fluids, 1, 171","venue":null,"work_id":"5e740e84-7a1f-4514-9be4-fdb730bf1ddd","year":1958},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.258128Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:c5b4f21892071a9aec186c6c318663304cb29cd3cef368a7e31593a1c11c8f2c","observation_id":"a599c50f-057a-4b7a-9324-c5497870c710","resolution":{"observed_at":"2026-08-14T11:25:44.775809Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.262101Z","title":null,"venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.262101Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:7c05b98efb47a5d33fc9c3844f26ab449a0c5f3cde9e44ab8397fac806f82593","observation_id":"51320902-7eb9-4757-b2c7-2a827e44b42d","resolution":{"observed_at":"2026-08-14T11:25:44.262101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.753641Z","title":"1978, Geophysical Journal, 54, 547","venue":null,"work_id":"76e11d3a-c5c9-42a6-b30b-e11cdc8ec214","year":1978},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.266037Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:027dd3469e7f384346024f39166406a1d561831a2791174233b5d9f61dfb1ccd","observation_id":"3638e941-e65e-4ec8-90d8-0a4d10d767bb","resolution":{"observed_at":"2026-08-14T11:25:44.757430Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.742047Z","title":"2010, SoPh, 267, 153","venue":null,"work_id":"e51890ef-1f39-4140-9299-6619d028d97c","year":2010},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.269573Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:f745f85f3878e76e0ca4f2809bef7b64f71c79770ed50d4fa908f15e6aea6112","observation_id":"df4706ba-408e-4bb4-a950-8343f0800055","resolution":{"observed_at":"2026-08-14T11:25:44.746699Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.731135Z","title":"2016, SoPh, 291, 2165","venue":null,"work_id":"2f407d34-374a-452d-aade-9e7a7c4527d1","year":2016},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.273232Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:bceebf6ad76b971822399655fc69e7f9e70706617600843e58ed60d8e7f2d56e","observation_id":"71491b80-4cae-4b6e-bc53-1ed89c373155","resolution":{"observed_at":"2026-08-14T11:25:44.734751Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.719242Z","title":"2001, Ap&SS, 277, 195","venue":null,"work_id":"f5b02aed-43cc-49f1-b226-f9f38b4c0e30","year":2001},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.276477Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:f7bb0f59b388ff610e8931e27dd684fe1872199c9dbb00c892e0a2b2ef992305","observation_id":"27f90eb3-4afe-49c4-98ca-e167d7ca0b46","resolution":{"observed_at":"2026-08-14T11:25:44.723113Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.707007Z","title":"G., Miggenrieder, H., M¨ uhlha¨ user, K.-H., et al","venue":null,"work_id":"983d3b37-e07b-4242-b9c0-625ce0346b21","year":1987},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.279866Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:3f859a27e1f0c37c483de2d7c1a3b4bddc39bdeb753488d68eb2c7049596872c","observation_id":"122a1590-be3f-47e4-99aa-c02c36778976","resolution":{"observed_at":"2026-08-14T11:25:44.711267Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.283528Z","title":"2014, Magnetohydrodynamics of the Sun (Cambridge University Press)","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.283528Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:9f87b8b76f4b84d9a39fa430220924be4a58aa5fe20f106610c1830219d24064","observation_id":"fd887258-5df1-47a9-a2b2-83bd02d2215f","resolution":{"observed_at":"2026-08-14T11:25:44.283528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.688749Z","title":"1998, ApJ, 500, 978","venue":null,"work_id":"7fcb6261-c261-4aa6-a038-f9ba0d31f717","year":1998},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.286987Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:31c500664cfaba729fdaeb7c8e2e73f4c4f6a288c47a62e3022101c0c5c9c8af","observation_id":"9013799e-7460-4b18-bef3-fa662a304d29","resolution":{"observed_at":"2026-08-14T11:25:44.692495Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.677751Z","title":null,"venue":null,"work_id":"1ab425e8-cfdf-4a9a-ad0b-2facd33cb7cd","year":2014},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.290298Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:3c14c63f9f4530674a5de295e2e83e7c8fea480eec20124b057420bd706198e1","observation_id":"412d0bd7-2920-4dbf-8f9f-b2f6b1e81315","resolution":{"observed_at":"2026-08-14T11:25:44.681376Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.667320Z","title":null,"venue":null,"work_id":"7329eb13-1b6a-4abe-91c1-5dd578bf795f","year":2017},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.293911Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:31954f21ef3f38778519083ab0156df94ecd59b46c1e7d51775fa29775960f0c","observation_id":"5e360fb1-bb68-4a2e-bff8-d772f44b0799","resolution":{"observed_at":"2026-08-14T11:25:44.671093Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.656738Z","title":null,"venue":null,"work_id":"3423f90a-ee76-4291-ba02-30c67646f6e8","year":2004},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.297214Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:a64a8e611dc1e328eb2ad1c4d30c7f816a6ec7348b4bacf170896b7d10924f74","observation_id":"ee5a1043-2b46-45c1-a6de-b5ca6f78d7ca","resolution":{"observed_at":"2026-08-14T11:25:44.660288Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.300370Z","title":null,"venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.300370Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:b40812ecda1d74e4b11fd060e14c1c33527aa24d642d91c40bfe574999aa53f2","observation_id":"a186a4c4-056f-480b-bd32-61e67fb4a206","resolution":{"observed_at":"2026-08-14T11:25:44.300370Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.639399Z","title":"H., & Soward, A","venue":null,"work_id":"95e55107-67fd-4009-a9ee-25b495f5c79d","year":1972},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.303820Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:96c1619882bca5f41161ab344962d894593659337756f63e4328fa6fdb9146b4","observation_id":"37e81ee6-8a89-4ae8-878c-aeb697510247","resolution":{"observed_at":"2026-08-14T11:25:44.642783Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.629457Z","title":"2011, Physics of Plasmas, 18, 012307","venue":null,"work_id":"057ee392-5f2c-450c-acce-1f9d63d79b59","year":2011},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.307160Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:e71d9552f4af832dc534d3f76e2f5cd96eae6d191b6881b41acfb3422f6efeca","observation_id":"a19b1973-421d-4cbc-a426-2f2d8db2ac82","resolution":{"observed_at":"2026-08-14T11:25:44.633068Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.618716Z","title":"S., Howes, G","venue":null,"work_id":"f18ee1ae-f877-41cc-9213-eb6831ca16ba","year":2012},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.310653Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:1385156750b9766b3fabe2cb000fef8608d3590bf5da7d3591ac4683720529d9","observation_id":"00d5a8eb-5060-41cf-af1d-08f64dd3a080","resolution":{"observed_at":"2026-08-14T11:25:44.622708Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.608238Z","title":"2017, The Astrophysical Journal, 835, 133","venue":null,"work_id":"75eebf7d-a7df-40b9-a298-c035a5e784d4","year":2017},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.314097Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:a0ce20274eaa9d4c8c0ebc664a2e99132a9bb80b6e3a89a3e58eaa65e6f68532","observation_id":"de8e02ae-25db-44ff-b436-9b64eca1aee7","resolution":{"observed_at":"2026-08-14T11:25:44.611803Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.596434Z","title":null,"venue":null,"work_id":"78d32dc1-1e7e-470d-b54b-f4095c0a2ed5","year":1975},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.317630Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:4300ffa6e6e84b0d960276566f696c2bb3222af0e0700439cef7cf8825e4d776","observation_id":"4f438933-3a80-4fa2-b43f-19ba0f7fae04","resolution":{"observed_at":"2026-08-14T11:25:44.600163Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.585416Z","title":"2017, Ap&SS, 362, 13","venue":null,"work_id":"15a4a1c8-ba58-4d07-a602-51166db4bc0f","year":2017},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.320938Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:48f58c59cafcff9c15b9bef60f2233018a2a9ae611225edadd5e82bfc230f86b","observation_id":"24b08d50-e5b4-4234-9f02-a9a3ef45457c","resolution":{"observed_at":"2026-08-14T11:25:44.589403Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.574685Z","title":null,"venue":null,"work_id":"640b07c5-9f40-4bd6-94bf-ece27b8fc3f5","year":2006},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.324406Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:f9d3892c7529d67a444e26a8968125f25119dc38e33969967a8a8b659797ad88","observation_id":"73076908-4706-4307-bcc8-e5cc2c8d1693","resolution":{"observed_at":"2026-08-14T11:25:44.578414Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.563700Z","title":"P., Goyal, R., Gaur, N., & Scime, E","venue":null,"work_id":"b8c9e0d8-5d6d-4e33-95c0-338025fb566b","year":2016},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.327814Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:db290ff24ed8b8ee33306e9ea1358ee479ba7e89597b6f92bf42aabcbd6284a0","observation_id":"164a58b4-57c0-431b-b825-2c599d88a895","resolution":{"observed_at":"2026-08-14T11:25:44.567444Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.552191Z","title":"B., Hammett, G","venue":null,"work_id":"5e67261d-413a-428a-9082-d863cc50aacd","year":1997},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.331199Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:ca6431b0a430c498858b705e652eea69ae0408cf192acac2db2e433d18e09345","observation_id":"37066d59-1ca7-4f67-9f4f-5a1fe4090cf2","resolution":{"observed_at":"2026-08-14T11:25:44.556116Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.540337Z","title":null,"venue":null,"work_id":"c213dbdb-0ac7-40fb-8b0e-53f43fa437d0","year":1992},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.334727Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:b97e03430d8fa0a95dad07023b48eef3cc27678f5ba8ed79bb8f73ec8a0efb4c","observation_id":"44cec88a-b666-4263-96bb-5058db545099","resolution":{"observed_at":"2026-08-14T11:25:44.544641Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.528367Z","title":"M., & Howes, G","venue":null,"work_id":"5ef5a3e9-f27b-4627-8a8f-d8269ada2ee1","year":2012},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.338476Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:c6c078d486539807d8fef0c2b0d6ec134031aa660ae3e15235ef64d8ff7d539c","observation_id":"e7e4c8c5-2e09-42fc-b342-82e5cbdcddb2","resolution":{"observed_at":"2026-08-14T11:25:44.532786Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.517968Z","title":"M., Howes, G","venue":null,"work_id":"f54da2be-fbc5-4ebd-a253-161c6944a198","year":2013},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.342329Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:551c4b17236526a9640c7e4560945819d1f0f7df1114413220ff2eda671df432","observation_id":"9b40c64d-9dd0-4f76-86aa-f3aabe250f70","resolution":{"observed_at":"2026-08-14T11:25:44.521301Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.506618Z","title":null,"venue":null,"work_id":"7bc1c0a9-d862-4dc8-8673-bf2a5aa8427e","year":2000},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.345880Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:7beccaf6ea8385a0739792140a61a21e2e6bf812dcc0fa7fe357af1f1012ead9","observation_id":"e87cba0d-d054-4e49-bf04-681689db692b","resolution":{"observed_at":"2026-08-14T11:25:44.510130Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.495342Z","title":null,"venue":null,"work_id":"78f47376-8cf3-44a3-b69e-e298af1623cf","year":2013},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.349293Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:9a26c72349089591d78b186c16ec9a3704d637bba8e97d185f49b45a222da891","observation_id":"e7a2ce9c-3181-42e9-96d0-6f529a643017","resolution":{"observed_at":"2026-08-14T11:25:44.498796Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.352990Z","title":null,"venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.352990Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:570a6087cae6f0cf09936c38260306bac76f6dd3902e997d1538fe06cbe5316e","observation_id":"ed139420-7f6f-474c-9f39-500103640836","resolution":{"observed_at":"2026-08-14T11:25:44.352990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.477232Z","title":"2010, The Astrophysical Journal, 719, 1335","venue":null,"work_id":"e381f08b-88e2-4aab-adfb-a0896788a380","year":2010},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.356638Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:144de9f22455aaf91a1debf4923c9ec3c9df72e771697ab270dd624ea054e508","observation_id":"ee0c4a6d-07b7-4ebf-8d19-4528f344e312","resolution":{"observed_at":"2026-08-14T11:25:44.481129Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.464702Z","title":"C., & Chang, C","venue":null,"work_id":"67843807-90ac-43e6-b787-3ba8a3a8a758","year":1965},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.360077Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:55673b761910277efe00e0a425d1fcd69652b6dddf279260c5238fabcb0a42b7","observation_id":"ed98cebc-b1ce-4784-8614-7e240e0e970c","resolution":{"observed_at":"2026-08-14T11:25:44.468718Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:25:44.451637Z","title":null,"venue":null,"work_id":"277833dc-04be-4b50-a96f-c802477e6062","year":2005},"citing_paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-14T11:25:44.363520Z"},"links":{"citing_paper":"/paper/1908.09198"},"observation_digest":"sha256:1beb2dabd4fd49bd5e65d03d10da4c22613b570e0300de76cf7af051643ef631","observation_id":"4675e48a-9f7d-476f-ab7b-919ebeea4594","resolution":{"observed_at":"2026-08-14T11:25:44.455613Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.09198","last_updated":"2019-08-24T20:27:50Z","latest_version":1,"primary_category":"physics.space-ph","snapshot_observed_at":"2026-08-16T02:23:01.125247Z","submitted_at":"2019-08-24T20:27:50Z","title":"Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":54,"verified_exact":0,"verified_fuzzy":46},"total_outbound_references":104},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 104 outbound references and 0 inbound Pith citation observations for arXiv:1908.09198."}