{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:CW4WTRT6N63NJ2TX5SCKFZP6XX","short_pith_number":"pith:CW4WTRT6","schema_version":"1.0","canonical_sha256":"15b969c67e6fb6d4ea77ec84a2e5febdea1cd90a0e98cab7dc4dd615ca6692a9","source":{"kind":"arxiv","id":"1701.00308","version":1},"attestation_state":"computed","paper":{"title":"\"Dandelion\" Filament Eruption and Coronal Waves Associated with a Solar Flare on 2011 February 16","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Ayumi Asai, Denis P. Cabezas, Jos\\'e K. Ishitsuka, Kazunari Shibata, Kenichi Otsuji, Lurdes M. Mart\\'inez, Mutsumi Ishitsuka, Reizaburo Kitai, Satoru UeNo, Satoshi Morita, Shinsuke Takasao, Takako T. Ishii, Yovanny J. Buleje, Yusuke Yoshinaga","submitted_at":"2017-01-02T02:37:47Z","abstract_excerpt":"Coronal disturbances associated with solar flares, such as H$\\alpha$ Moreton waves, X-ray waves, and extreme ultraviolet (EUV) coronal waves are discussed herein in relation to magnetohydrodynamics fast-mode waves or shocks in the corona. To understand the mechanism of coronal disturbances, full-disk solar observations with high spatial and temporal resolution over multiple wavelengths are of crucial importance. We observed a filament eruption, whose shape is like a \"dandelion\", associated with the M1.6 flare that occurred on 2011 February 16 in the H$\\alpha$ images taken by the Flare Monitori"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1701.00308","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-01-02T02:37:47Z","cross_cats_sorted":[],"title_canon_sha256":"23147bbd8afef71bb93b8a25c345524237ba581bf4fb07e56f10995b82d317c2","abstract_canon_sha256":"92d870ebff9e1db57ea48e4e488e4193f9289a9ced4488daa55ad81a77c44495"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:46.021830Z","signature_b64":"9Sc2yyOeEs8wgpG5keCwPn7Hd4vpqP98YMHD64wlPW1Zs/oiIsZHyvP2LBF8z3cLD2vlQWiOcVqbwkYuIaFKDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"15b969c67e6fb6d4ea77ec84a2e5febdea1cd90a0e98cab7dc4dd615ca6692a9","last_reissued_at":"2026-05-18T00:50:46.021083Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:46.021083Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"\"Dandelion\" Filament Eruption and Coronal Waves Associated with a Solar Flare on 2011 February 16","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Ayumi Asai, Denis P. Cabezas, Jos\\'e K. Ishitsuka, Kazunari Shibata, Kenichi Otsuji, Lurdes M. Mart\\'inez, Mutsumi Ishitsuka, Reizaburo Kitai, Satoru UeNo, Satoshi Morita, Shinsuke Takasao, Takako T. Ishii, Yovanny J. Buleje, Yusuke Yoshinaga","submitted_at":"2017-01-02T02:37:47Z","abstract_excerpt":"Coronal disturbances associated with solar flares, such as H$\\alpha$ Moreton waves, X-ray waves, and extreme ultraviolet (EUV) coronal waves are discussed herein in relation to magnetohydrodynamics fast-mode waves or shocks in the corona. To understand the mechanism of coronal disturbances, full-disk solar observations with high spatial and temporal resolution over multiple wavelengths are of crucial importance. We observed a filament eruption, whose shape is like a \"dandelion\", associated with the M1.6 flare that occurred on 2011 February 16 in the H$\\alpha$ images taken by the Flare Monitori"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.00308","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1701.00308","created_at":"2026-05-18T00:50:46.021204+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.00308v1","created_at":"2026-05-18T00:50:46.021204+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.00308","created_at":"2026-05-18T00:50:46.021204+00:00"},{"alias_kind":"pith_short_12","alias_value":"CW4WTRT6N63N","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"CW4WTRT6N63NJ2TX","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"CW4WTRT6","created_at":"2026-05-18T12:31:10.602751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX","json":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX.json","graph_json":"https://pith.science/api/pith-number/CW4WTRT6N63NJ2TX5SCKFZP6XX/graph.json","events_json":"https://pith.science/api/pith-number/CW4WTRT6N63NJ2TX5SCKFZP6XX/events.json","paper":"https://pith.science/paper/CW4WTRT6"},"agent_actions":{"view_html":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX","download_json":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX.json","view_paper":"https://pith.science/paper/CW4WTRT6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.00308&json=true","fetch_graph":"https://pith.science/api/pith-number/CW4WTRT6N63NJ2TX5SCKFZP6XX/graph.json","fetch_events":"https://pith.science/api/pith-number/CW4WTRT6N63NJ2TX5SCKFZP6XX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX/action/storage_attestation","attest_author":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX/action/author_attestation","sign_citation":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX/action/citation_signature","submit_replication":"https://pith.science/pith/CW4WTRT6N63NJ2TX5SCKFZP6XX/action/replication_record"}},"created_at":"2026-05-18T00:50:46.021204+00:00","updated_at":"2026-05-18T00:50:46.021204+00:00"}