{"as_of":"2026-08-14T20:39:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:13363cdcf7adaf2a563ffba88644cc58ee0ec69c18fc52725aa9adb66af7c36c","coverage":[{"denominator":72,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":72,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T01:30:35.807806Z","state":"measured"},{"denominator":72,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":72,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+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/2607.25799/citation-record","integrity":"/paper/2607.25799/integrity","json":"/paper/2607.25799/citation-record.json","paper":"/paper/2607.25799"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T01:30:32.769782Z","title":"Chinese Journal of Space Science2025;45: 913–942","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:32.769782Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:530eb1a9f2574b1b285b74871bdefff3a533d0d6c15e3ede5d4a82ff79d2749e","observation_id":"636d7fc6-2340-43d9-81eb-77e376f3f339","resolution":{"observed_at":"2026-08-01T01:30:32.769782Z","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":"2026-08-01T01:30:32.832228Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:32.832228Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:8df485cb368f8ab1fd72a8c75ad4dc8d72108583ef0947428982ea69323a77d5","observation_id":"2db8a86a-b62c-49a8-8dc8-ffe0f5b481a2","resolution":{"observed_at":"2026-08-01T01:30:32.832228Z","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":"2026-08-01T01:30:32.902347Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:32.902347Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:2b7ca6778a29e58464d9721a29dae0243b25b826ce2564d3eca2496f04d519b4","observation_id":"51484392-3584-4caa-8509-2a1a334cb427","resolution":{"observed_at":"2026-08-01T01:30:32.902347Z","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":"2026-08-01T01:30:32.970056Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:32.970056Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:a4530d68830fc0ec8a6c1a18132c7691f13235cc1ab974fa82b02996155f32e7","observation_id":"960fa4ec-8390-4242-8768-fa74516ec522","resolution":{"observed_at":"2026-08-01T01:30:32.970056Z","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":"2026-08-01T01:30:33.036431Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.036431Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:f46c2153eef10bae520696cfc2cf73fca38bc6b3105485f2600f7dbdfc09decc","observation_id":"ea59acf0-6ae2-4e40-9a6e-e077adec1739","resolution":{"observed_at":"2026-08-01T01:30:33.036431Z","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":"2026-08-01T01:30:33.105956Z","title":"The effects of high-frequency Alfven waves on coronal heating and solar wind acceleration.As- tronomy and Astrophysics1997;319: L17–L20","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.105956Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:d2cea865be2d19074e86280cb727690c37a9da4048da56cbe8aebee792f1d128","observation_id":"0bbcd159-544d-4952-ae70-cd28231649de","resolution":{"observed_at":"2026-08-01T01:30:33.105956Z","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":"2026-08-01T01:30:33.252301Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.252301Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:60289d9cd3bb28ccbc9ae96fa993229a7d45b7a73ef42f6f8f7fe1994b64403a","observation_id":"d5406750-7052-4213-a773-cc608188deec","resolution":{"observed_at":"2026-08-01T01:30:33.252301Z","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":"2026-08-01T01:30:33.292950Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.292950Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:0513c33bb292ecfb425beb76c481a6eadfd578fad25aa88cabe5721d7f4eadfe","observation_id":"dbbd4677-8e02-4ad0-a233-b5ebc2d2c124","resolution":{"observed_at":"2026-08-01T01:30:33.292950Z","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":"2026-08-01T01:30:33.354837Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.354837Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:4c8d2ccec9cdb62e19206f17e005f39c1dbe001889dacddce499463a3d1928a4","observation_id":"2bd6d916-84c3-493c-b35e-d6aed34ccc9c","resolution":{"observed_at":"2026-08-01T01:30:33.354837Z","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":"2026-08-01T01:30:33.425012Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.425012Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:ab863e8a73b0040acc187bf7b0cbddab8685a4bfeb63a61f5413c9ba8076bf80","observation_id":"b39ef29a-cd06-4a55-8e7a-66d80fc2b604","resolution":{"observed_at":"2026-08-01T01:30:33.425012Z","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":"2026-08-01T01:30:33.495163Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.495163Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:b4587fe1e31a643db739918b0f219631571142fa210eb5b2e56b68ac9e0377db","observation_id":"daded6f3-57a1-46fc-b6f6-7802f452b305","resolution":{"observed_at":"2026-08-01T01:30:33.495163Z","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":"2026-08-01T01:30:33.535149Z","title":"First Direct Measurements of Transverse Waves in Solar Polar Plumes Using SDO/AIA.the Astrophysical Journal Letters2014; 790:L2","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.535149Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:fd042a863d55e331d71294627d11f06d95416b1524a372eec743f7f754415079","observation_id":"12be7583-07f4-4b01-b467-b03c336ca98e","resolution":{"observed_at":"2026-08-01T01:30:33.535149Z","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":"2026-08-01T01:30:33.638062Z","title":"Investigating Alfv ´enic wave propagation in coronal open-field regions.Nature Communications2015;6:7813","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.638062Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:63c87268c828c9af1c6c756c5daa7babd77a3fb0dbb513a84be9b3136d4cc403","observation_id":"6d458d12-ded9-44af-9a32-0743d71a9d94","resolution":{"observed_at":"2026-08-01T01:30:33.638062Z","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":"2026-08-01T01:30:33.707700Z","title":"A basal contri- bution from p-modes to the Alfv ´enic wave flux in the Sun’s corona.Nature Astronomy2019;3: 223","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.707700Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:8d2067585d7c7243d859c7a54500074c6cefa6f4b48a3e1f4365e1bc038cea71","observation_id":"c5005a34-246e-41b6-b24a-b8710c1f4ed3","resolution":{"observed_at":"2026-08-01T01:30:33.707700Z","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":"2026-08-01T01:30:33.767775Z","title":"Using Trans- verse Waves to Probe the Plasma Conditions at the Base of the Solar Wind.the Astrophysical Journal2020;894:79","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.767775Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:e22f31ae2d2526d0b903bdfa37ca2c1e3cfb04e0df905dc053f87434aa7c1bab","observation_id":"73adc19b-615f-46d0-b3f8-8204e6a22158","resolution":{"observed_at":"2026-08-01T01:30:33.767775Z","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":"2026-08-01T01:30:33.829773Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.829773Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:8ea00c386556a3f7a64d149ddb1a9274a6f88a9436e23ee247d39c858c45a2e9","observation_id":"4e0414b7-5b22-4bda-93df-193f1894ea27","resolution":{"observed_at":"2026-08-01T01:30:33.829773Z","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":"2026-08-01T01:30:33.887777Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.887777Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:5614db805d24d6f6ad86fac894e3b8b34391afcab5a0361acc71bfb6bf154aa1","observation_id":"71b47def-0959-4c60-87bd-2cb9566feaf0","resolution":{"observed_at":"2026-08-01T01:30:33.887777Z","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":"2026-08-01T01:30:33.946812Z","title":"Science2024;386: 76–82","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.946812Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:4415c850c28f6f3a69e05fe1a77f888c632801847fbb2de7d155f4478a7df00f","observation_id":"ac42dc97-cf9e-4369-ad9c-ad76168f5967","resolution":{"observed_at":"2026-08-01T01:30:33.946812Z","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":"2026-08-01T01:30:33.992883Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:33.992883Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:500388cbcc7f6356bff7bb35e69be0414697222688942a63844a9330644a81cd","observation_id":"1c624316-328b-403f-bac8-65e7424eb94c","resolution":{"observed_at":"2026-08-01T01:30:33.992883Z","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":"2026-08-01T01:30:34.048004Z","title":"An Automated Algorithm for Identifying and Tracking Transverse Waves in Solar Images.the Astrophysical Journal2018;852:57","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.048004Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:3407fdd71f9092a1331fd6c43c38779652dda46e048191eb3dc061c839690190","observation_id":"b6d72980-bb39-491f-bbdc-931353828c44","resolution":{"observed_at":"2026-08-01T01:30:34.048004Z","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":"2026-08-01T01:30:34.109095Z","title":"Selective spatial damping of propagating kink waves due to resonant ab- sorption.Astronomy and Astrophysics2010;524:A23","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.109095Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:eded483f782ae193372993644c2b2713d6b61c9777825539f84378b02c28f629","observation_id":"099890ab-d8b5-4c3d-9caf-7e5891166525","resolution":{"observed_at":"2026-08-01T01:30:34.109095Z","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":"2026-08-01T01:30:34.171207Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.171207Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:18a89eb8e92b8b64fa6dfeb4573ecd04469178fcd00f4437f267bf20be77a058","observation_id":"06d484f9-f8d4-4a44-89f4-90c66221f5e0","resolution":{"observed_at":"2026-08-01T01:30:34.171207Z","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":"2026-08-01T01:30:34.238467Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.238467Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:0a37bea0163956b941df8d164ab1a6084617db2cf82e12cc295096b1bc1a55c5","observation_id":"7cb03460-6294-4e3b-86a6-651180264e26","resolution":{"observed_at":"2026-08-01T01:30:34.238467Z","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":"2026-08-01T01:30:34.277564Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.277564Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:d781c4557e75eca27bb996af10ef86344b5ba46267febee78799c6c665e26916","observation_id":"f46ecd2a-9213-4fe3-8a7e-9711742ec723","resolution":{"observed_at":"2026-08-01T01:30:34.277564Z","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":"2026-08-01T01:30:34.323685Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.323685Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:7b81a44a1a3c3e7deb8c796027e3bb8db6b9e4483901e25aa81390b2bd5f6a65","observation_id":"89396239-23cc-4041-9928-dcf183c7eda2","resolution":{"observed_at":"2026-08-01T01:30:34.323685Z","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":"2026-08-01T01:30:34.347555Z","title":"Science overview.Astronomy and Astrophysics 2020;642:A1","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.347555Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:a94809490c96a2204c4d3c1e08da6ee4fceeaffc6079c211f4281732dadcc089","observation_id":"3cc0121c-6b16-49e3-a272-c62b435be6c8","resolution":{"observed_at":"2026-08-01T01:30:34.347555Z","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":"2026-08-01T01:30:34.388638Z","title":"Solar Coronal Plumes.Living Reviews in Solar Physics2015;12:7","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.388638Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:056b514adf713dd65de9b1daf0544b1abe73bcf157fa252759ad12c2cd8f74c7","observation_id":"1aeb1c93-bc29-4fa0-a563-dc592fd39e68","resolution":{"observed_at":"2026-08-01T01:30:34.388638Z","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":"2026-08-01T01:30:34.421811Z","title":"the Astrophysical Journal Letters2025;991:L45","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.421811Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:d61136a08be1223dadf60685ca4bb5d59a0a31ab00d53322722c09568de073e8","observation_id":"3c50b73b-cc4c-4611-a202-57b0a7a58cbf","resolution":{"observed_at":"2026-08-01T01:30:34.421811Z","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":"2026-08-01T01:30:34.463479Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.463479Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:1e7d7f09068b7425c5292953729cbfc2d9d5c0ecbea711e9277ad9b636233575","observation_id":"266eb5b0-418c-4214-b349-99b30c6e035e","resolution":{"observed_at":"2026-08-01T01:30:34.463479Z","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":"2026-08-01T01:30:34.519175Z","title":"The Solar Dynamics Observatory (SDO).Solar Physics2012;275: 3–15","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.519175Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:201e5e307858ab9d35352c5011403c575a4ee43534d679c1129f4201b422ede3","observation_id":"c3ab898b-9de9-4956-8559-929db6579e34","resolution":{"observed_at":"2026-08-01T01:30:34.519175Z","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":"2026-08-01T01:30:34.580129Z","title":"On the Origins of Coronal Alfv ´enic Waves.the Astrophysical Journal Letters2025;986:L6","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.580129Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:535ac166e981d66e81f847c147eef0a118b93fc197c54c2b0deb77a376ccd29b","observation_id":"4b08fdc7-3f78-40f4-93d0-22e5efe6a116","resolution":{"observed_at":"2026-08-01T01:30:34.580129Z","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":"2026-08-01T01:30:34.640357Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.640357Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:705380a96592129f775b1fe6b3333fb7ba698d88fd5111b28e99582ef64d305a","observation_id":"80ec75fe-c43c-4088-8983-bc64987fef6d","resolution":{"observed_at":"2026-08-01T01:30:34.640357Z","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":"2026-08-01T01:30:34.685728Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.685728Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:d5e49cf71604efb28c34df5b8c26db23a5ac7caa99fd4f75621d67da69c8a1f4","observation_id":"dca0e4c9-9f50-46f0-8c89-58ea9cdb61dc","resolution":{"observed_at":"2026-08-01T01:30:34.685728Z","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":"2026-08-01T01:30:34.727756Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.727756Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:25e3bda2e30dc2b4bde1f272f17db306320db88225735d0aba1bffe426bea7ae","observation_id":"4195ce0d-b7c9-4943-98d8-a9b29421381f","resolution":{"observed_at":"2026-08-01T01:30:34.727756Z","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":"2026-08-01T01:30:34.767802Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.767802Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:3d9fef04cb0542f5194c3602b8f6b0084bbeee0ff77db28614a548b0578024bb","observation_id":"4dbd0bc1-2203-427b-bb51-ae6b57fac389","resolution":{"observed_at":"2026-08-01T01:30:34.767802Z","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":"2026-08-01T01:30:34.809772Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.809772Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:3537faa6659eaf0a9540198ad34918043b9cbae8f64e868d662eb358f331a774","observation_id":"ccd02858-0b4e-46b8-8901-a038a6ba8aed","resolution":{"observed_at":"2026-08-01T01:30:34.809772Z","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":"2026-08-01T01:30:34.853026Z","title":"Interchange Recon- nection Alfv´en Wave Generation.Solar Physics2014;289: 3043–3058","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.853026Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:5c1a478368e36126a427b51077bb0ed64fd2092c13471d489803ab3d0f26513e","observation_id":"5657d428-2bb8-4bf2-b2e4-bd2006f6d97b","resolution":{"observed_at":"2026-08-01T01:30:34.853026Z","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":"2026-08-01T01:30:34.894280Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.894280Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:1423bc2faae0594f70a3539a036553e23c4bc075f1cedafc2bb2d20f75b1664c","observation_id":"3d6799b9-33b1-46e1-83b1-38ca3b16d27b","resolution":{"observed_at":"2026-08-01T01:30:34.894280Z","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":"2026-08-01T01:30:34.945280Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:34.945280Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:77f0f4c2e448d4cdc352a2c1a6d7db89ce22baa2027ddae118cff7c71025c96b","observation_id":"91e9b758-5379-42de-805e-ba2d6cd22bc7","resolution":{"observed_at":"2026-08-01T01:30:34.945280Z","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":"2026-08-01T01:30:35.003085Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.003085Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:4cb99592baf7f0cb7e1f5e2596f4fd11d1f9f157964d140454366eda7ebeeb47","observation_id":"1db207b4-3d7c-47d3-bfeb-2fe95d36a3c3","resolution":{"observed_at":"2026-08-01T01:30:35.003085Z","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":"2026-08-01T01:30:35.057310Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.057310Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:6272d377f46f2d0ec42f7b3d8988becc13d52f63ab4ac273e0a9d34be1fb165b","observation_id":"9705f10e-38ff-4cb3-894f-0fe74c968c50","resolution":{"observed_at":"2026-08-01T01:30:35.057310Z","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":"2026-08-01T01:30:35.117996Z","title":"Propagating Distur- bances in the Solar Corona and Spicular Connection.the Astrophysical Journal Letters2015;815:L16","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.117996Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:e601d597956ab16e66ec1c683cb0569d99e119437dd9e410dbcddefd393b36af","observation_id":"17f3ee59-a8f2-48b7-b653-18d711a8cdae","resolution":{"observed_at":"2026-08-01T01:30:35.117996Z","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":"2026-08-01T01:30:35.205420Z","title":"the Astrophysical Journal2026;1001:173","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.205420Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:a3e35039ae37105b1555be1df10c02d4ed39579c63d4a1ad027d3cbd8b262878","observation_id":"e6f7f8c2-1423-4e93-9243-52a3e319d3ae","resolution":{"observed_at":"2026-08-01T01:30:35.205420Z","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":"2026-08-01T01:30:35.237486Z","title":"Observations of counter- propagating Alfv ´enic and compressive fluctuations in the chromosphere.Research in Astronomy and Astrophysics 2014;14:299-310","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.237486Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:d9bd377798414d7ea25a40057a6effc965626914c6b05cf185b9c471b6b6fffa","observation_id":"0d92fc66-5068-45ec-a3d6-4fd36203d412","resolution":{"observed_at":"2026-08-01T01:30:35.237486Z","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":"2026-08-01T01:30:35.306961Z","title":"Gener- alized phase mixing: Turbulence-like behaviour from uni- directionally propagating MHD waves.Scientific Reports 2017;7:14820","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.306961Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:76a30ad4c1491a31ffd5a775a6462180a73c842b2b96f3e2ae6da43b4d680c4b","observation_id":"fbb11574-9a67-4c38-9b84-1a085369b57c","resolution":{"observed_at":"2026-08-01T01:30:35.306961Z","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":"2026-08-01T01:30:35.356052Z","title":"Mode conversion and energy flux absorption in the structured solar atmosphere","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.356052Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:6925a2e5852fcda3e7fc42b5904a2e788e6dd9206f17a8de9d18dfa023f512b0","observation_id":"555f43e8-a00c-4faf-979b-69865a7d0a61","resolution":{"observed_at":"2026-08-01T01:30:35.356052Z","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":"2026-08-01T01:30:35.399964Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.399964Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:45b132b9e800fe3f2d16617168f7105d70232b19dd58506bb2172c1bab9335cc","observation_id":"2243ce55-4751-45b3-a4ec-28de3d1888ee","resolution":{"observed_at":"2026-08-01T01:30:35.399964Z","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":"2026-08-01T01:30:35.469148Z","title":"High-frequency Spicule Oscil- lations Generated via Mode Conversion.the Astrophysical Journal2018;854:9","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.469148Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:21b88c4db2b331ce7f5f00ff4edb4ee81b080d04a4832b05bccc1119a5cd1a41","observation_id":"0e4fd0ec-e3c6-4b45-9c04-fd69c65e4b03","resolution":{"observed_at":"2026-08-01T01:30:35.469148Z","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":"2026-08-01T01:30:35.511229Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.511229Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:0bc184678064aba1ba9985b5ec1397d96c07c17ccee47748674125a83f42d9b8","observation_id":"556ce0e9-8ad9-4fe3-9196-ed49d14b4f62","resolution":{"observed_at":"2026-08-01T01:30:35.511229Z","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":"2026-08-01T01:30:35.557349Z","title":"Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter.Solar Physics2023;298:5","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.557349Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:ff5247a956650e622f08883414a58dac6197ec2c73f20c8d17b4746b19d50470","observation_id":"f0c4015b-5bc6-4a36-be72-a5843c5809cf","resolution":{"observed_at":"2026-08-01T01:30:35.557349Z","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":"2026-08-01T01:30:35.633535Z","title":"Inouye Solar Telescope - Observatory Overview.Solar Physics 2020;295:172","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.633535Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:f5b7495eaa9dab440dee31a013ec9147b96f33ab9c629d7e6e30552c02086c4f","observation_id":"b38faadb-ab56-4b3a-a848-c638f97158f1","resolution":{"observed_at":"2026-08-01T01:30:35.633535Z","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":"2026-08-01T01:30:35.682657Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.682657Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:fdc5eee04b26d7ac95573b2e49c58048fe5678b5177c7b77e9d29b1b9e7e413f","observation_id":"a0b7c4c7-5bd9-46a8-ab45-dbf453dfe16a","resolution":{"observed_at":"2026-08-01T01:30:35.682657Z","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":"2026-08-01T01:30:35.706409Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.706409Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:fc60606f9c9424ee9ad3772a52d59c7b850120158af50f310702d77ec6d0c460","observation_id":"ca5a8532-5608-42a0-a226-39f68944f56d","resolution":{"observed_at":"2026-08-01T01:30:35.706409Z","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":"2026-08-01T01:30:35.740033Z","title":"Heating of the Magnetized Solar Chromosphere by Partial Ionization Effects.the As- trophysical Journal2012;747:87","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.740033Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:1aec3b07a5a6a34864ce7f6f2e5360659a2ff9d2e1501185028a3c0c908726ac","observation_id":"8699635e-f2df-4cee-9efa-8920d57bb8db","resolution":{"observed_at":"2026-08-01T01:30:35.740033Z","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":"2026-08-01T01:30:35.756809Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.756809Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:ad000a384aa24d82041276a41d5b69224a7067b2d90cc12cbb2f4e7b9bbd9d4e","observation_id":"f2b8e375-a3e0-4865-a55e-6ad4ac725c43","resolution":{"observed_at":"2026-08-01T01:30:35.756809Z","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":"2026-08-01T01:30:35.760118Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.760118Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:8bac179fda39987b0fec9370395dd48aa040494e2b4f759607a1957170140923","observation_id":"83efd534-c9c3-42b2-85c6-97914b45d90a","resolution":{"observed_at":"2026-08-01T01:30:35.760118Z","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":"2026-08-01T01:30:35.763052Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.763052Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:bed88a645c262625815119a9a2d8975b13930aea3436396932bed3ab05c2a24a","observation_id":"d22109c5-de92-47d3-bd8c-ab698b95ab99","resolution":{"observed_at":"2026-08-01T01:30:35.763052Z","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":"2026-08-01T01:30:35.765919Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.765919Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:5b0fac1383c49af81d4dd5152286e934de601551d15b84d1b56fa6ea5808faf0","observation_id":"1b4cc985-d956-4084-8270-74ad78f3f5a1","resolution":{"observed_at":"2026-08-01T01:30:35.765919Z","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":"2026-08-01T01:30:35.768716Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.768716Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:9a81b37c835844a4b77554594a7b55fd475a9fb91e721f519847775ce763c06d","observation_id":"31c70821-118d-4286-82b1-f3f97ff40144","resolution":{"observed_at":"2026-08-01T01:30:35.768716Z","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":"2026-08-01T01:30:35.771545Z","title":"Coronal Cells in Coronal Holes: Systematic Analysis and Implications for Coronal Evolution.the Astrophysical Journal2025;991:55","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.771545Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:76d6a245f7127c8ccdcfaa065cd863718163b977eceb965558b2e973e1d083bc","observation_id":"cfae69aa-4622-477a-83c1-7753a4e6ccb2","resolution":{"observed_at":"2026-08-01T01:30:35.771545Z","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":"2026-08-01T01:30:35.774699Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.774699Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:26277d1333835471fe6149883433a26375968eb2fa0e3b69b4929f2dade30ea2","observation_id":"fc953bfa-3752-4243-aca7-7660ccad2dfd","resolution":{"observed_at":"2026-08-01T01:30:35.774699Z","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":"2026-08-01T01:30:35.777836Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.777836Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:5febb7be1b0798628e96b8de8b19982af3443986e23b63eef0d026129c013d3d","observation_id":"cf3b7891-0b29-405c-a648-a15724f51afe","resolution":{"observed_at":"2026-08-01T01:30:35.777836Z","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":"2026-08-01T01:30:35.780879Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.780879Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:4697ad77bfee6471286acdab3fae6097cfa720990c95ffa2df2e2e8fc66b47f6","observation_id":"5b5a545c-8514-4450-b59a-b6993a0e41cf","resolution":{"observed_at":"2026-08-01T01:30:35.780879Z","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":"2026-08-01T01:30:35.783876Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.783876Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:5b2956bc2385a449c27cc2e6c209d9c30beeec060ef57a2c7fb72153bf8b992a","observation_id":"918a4b2d-9a1b-4882-8b88-62462b1615e3","resolution":{"observed_at":"2026-08-01T01:30:35.783876Z","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":"2026-08-01T01:30:35.786567Z","title":"Resonant MHD Waves in the Solar Atmosphere.Space Science Reviews 2011;158: 289–338","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.786567Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:915b2148c17d31980df18a4950314648be5a5f7a24298c8f3f34033016401938","observation_id":"5ebfa8c9-b81b-4371-b60b-8b7c2556477e","resolution":{"observed_at":"2026-08-01T01:30:35.786567Z","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":"2026-08-01T01:30:35.789428Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.789428Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:acd0b46e19620d477f68dd5d5c3c806b694bba936d2b243df87858a7f3159ca1","observation_id":"9fd0e5f2-6147-4e1b-b004-f4c4abeb71da","resolution":{"observed_at":"2026-08-01T01:30:35.789428Z","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":"2026-08-01T01:30:35.792367Z","title":"Contribution of observed multi frequency spectrum of Alfv´en waves to coronal heating.As- tronomy and Astrophysics2019;623:A37","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.792367Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:1f33db266bda98daf9008f0aca0562be036679983a9b4ddc735a9216a2979a3d","observation_id":"9e0a0d7f-9825-4d0e-b0d1-7a3a04c44820","resolution":{"observed_at":"2026-08-01T01:30:35.792367Z","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":"2026-08-01T01:30:35.795556Z","title":"Investigating Sub-Pixel 45- Second Periodic Wobble in SDO/AIA Data from January to August 2012.Solar Physics2018;293:147","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.795556Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:bc9071614148bb046cd6fcc6417e398b24f2a9da9221736b2bea9c8885687433","observation_id":"9e50351c-1e90-4308-8bcf-d883b7a93a0d","resolution":{"observed_at":"2026-08-01T01:30:35.795556Z","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":"2026-08-01T01:30:35.798759Z","title":"Noise-gating to Clean Astrophysical Image Data.the Astrophysical Journal2017;838:155","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.798759Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:81c6e9859c85f7429b4bfda7d85b41350d87e8d6134dd044f6dd3094fe4f9788","observation_id":"d91813f4-1461-47e7-9ecc-696bcb34318d","resolution":{"observed_at":"2026-08-01T01:30:35.798759Z","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":"2026-08-01T01:30:35.801987Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.801987Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:e4f8bbe18cc1c013e46030d2b3e979330eae119cf249cab1cc3748259409dd3c","observation_id":"5c1aaea3-d77d-43a6-8b53-a1b4e01a3424","resolution":{"observed_at":"2026-08-01T01:30:35.801987Z","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":"2026-08-01T01:30:35.804955Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.804955Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:fadf9f2439184074ee7741a74773e9a0f7699e584cc32783186c76edda75e478","observation_id":"2a86adce-aba0-4b24-99a3-0e5318d2ee4a","resolution":{"observed_at":"2026-08-01T01:30:35.804955Z","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":"2026-08-01T01:30:35.807806Z","title":"Revisiting the Relation be- tween Nonthermal Line Widths and Transverse MHD Wave Amplitudes.the Astrophysical Journal2020;899:1","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-01T01:30:35.807806Z"},"links":{"citing_paper":"/paper/2607.25799"},"observation_digest":"sha256:e920d4d7aaa855ef4facd52481740d45f4e174f68d5de230ab65eaee56ca38a7","observation_id":"3d3d9e54-04d0-47b6-b53d-4aaa3ad0052d","resolution":{"observed_at":"2026-08-01T01:30:35.807806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.25799","last_updated":"2026-07-28T14:47:28Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-10T06:44:26.488797Z","submitted_at":"2026-07-28T14:47:28Z","title":"High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona"},"reference_resolution":{"displayed":72,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":72,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":72},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 72 of 72 outbound references and 0 inbound Pith citation observations for arXiv:2607.25799."}