{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:V5QOQBWAXPUYDWKQ55TM3W2P53","short_pith_number":"pith:V5QOQBWA","schema_version":"1.0","canonical_sha256":"af60e806c0bbe981d950ef66cddb4feedc8bb064f6aa0f231929eeb0f226029f","source":{"kind":"arxiv","id":"2305.11691","version":1},"attestation_state":"computed","paper":{"title":"EUV fine structure and variability associated with coronal rain revealed by Solar Orbiter/EUI HRIEUV and SPICE","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. Dolliou, A. N. Zhukov, C. Verbeeck, D. Berghmans, D. M. Long, E. Buchlin, E. Kraaikamp, F. Auch\\`ere, F. Delmotte, G. Aulanier, H. Peter, J.-F. Hochedez, J. M. Gilles, J.-P. Halain, K. Barczynski, K. Heerlein, K. Stegen, L. Harra, L. P. Chitta, L. Rodriguez, L. Teriaca, M. Gyo, M. Haberreiter, M. Janvier, M. J. West, P. Antolin, P. J. Smith, P. Rochus, R. Aznar Cuadrado, S. Gissot, S. K. Solanki, S. Mandal, S. Parenti, S. Poedts, T. Appourchaux, U. Sch\\\"uhle, Z. Huang","submitted_at":"2023-05-19T14:13:25Z","abstract_excerpt":"Coronal rain is the most dramatic cooling phenomenon of the solar corona and an essential diagnostic tool for the coronal heating properties. A puzzling feature of the solar corona, besides the heating, is its EUV filamentary structure and variability. We aim to identify observable features of the TNE-TI scenario underlying coronal rain at small and large spatial scales, to understand the role it plays in the solar corona. We use EUV datasets at unprecedented spatial resolution of ~240 km from EUI/HRIEUV and SPICE of Solar Orbiter from the spring 2022 perihelion. EUV absorption features produc"},"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":"2305.11691","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2023-05-19T14:13:25Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"80a9b5e103be8057bd9e27d792d188766c73d51413b2ae5489781c2f5e52c377","abstract_canon_sha256":"ae4d0e92008fc87597b0508d4c0bdd513d5c963513f2a3b3c77f1838c87ab747"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:43:38.975578Z","signature_b64":"sqNFfPzH51fu4ZcBnBg7aY3GLCGfoJ+DTh+3wFQsDgvR72OrUA8Kf5IfMOCHsdlvOh2A2yopOkBLh33phHBRCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"af60e806c0bbe981d950ef66cddb4feedc8bb064f6aa0f231929eeb0f226029f","last_reissued_at":"2026-07-05T06:43:38.975090Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:43:38.975090Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"EUV fine structure and variability associated with coronal rain revealed by Solar Orbiter/EUI HRIEUV and SPICE","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. Dolliou, A. N. Zhukov, C. Verbeeck, D. Berghmans, D. M. Long, E. Buchlin, E. Kraaikamp, F. Auch\\`ere, F. Delmotte, G. Aulanier, H. Peter, J.-F. Hochedez, J. M. Gilles, J.-P. Halain, K. Barczynski, K. Heerlein, K. Stegen, L. Harra, L. P. Chitta, L. Rodriguez, L. Teriaca, M. Gyo, M. Haberreiter, M. Janvier, M. J. West, P. Antolin, P. J. Smith, P. Rochus, R. Aznar Cuadrado, S. Gissot, S. K. Solanki, S. Mandal, S. Parenti, S. Poedts, T. Appourchaux, U. Sch\\\"uhle, Z. Huang","submitted_at":"2023-05-19T14:13:25Z","abstract_excerpt":"Coronal rain is the most dramatic cooling phenomenon of the solar corona and an essential diagnostic tool for the coronal heating properties. A puzzling feature of the solar corona, besides the heating, is its EUV filamentary structure and variability. We aim to identify observable features of the TNE-TI scenario underlying coronal rain at small and large spatial scales, to understand the role it plays in the solar corona. We use EUV datasets at unprecedented spatial resolution of ~240 km from EUI/HRIEUV and SPICE of Solar Orbiter from the spring 2022 perihelion. EUV absorption features produc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.11691","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2305.11691/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2305.11691","created_at":"2026-07-05T06:43:38.975142+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.11691v1","created_at":"2026-07-05T06:43:38.975142+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.11691","created_at":"2026-07-05T06:43:38.975142+00:00"},{"alias_kind":"pith_short_12","alias_value":"V5QOQBWAXPUY","created_at":"2026-07-05T06:43:38.975142+00:00"},{"alias_kind":"pith_short_16","alias_value":"V5QOQBWAXPUYDWKQ","created_at":"2026-07-05T06:43:38.975142+00:00"},{"alias_kind":"pith_short_8","alias_value":"V5QOQBWA","created_at":"2026-07-05T06:43:38.975142+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/V5QOQBWAXPUYDWKQ55TM3W2P53","json":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53.json","graph_json":"https://pith.science/api/pith-number/V5QOQBWAXPUYDWKQ55TM3W2P53/graph.json","events_json":"https://pith.science/api/pith-number/V5QOQBWAXPUYDWKQ55TM3W2P53/events.json","paper":"https://pith.science/paper/V5QOQBWA"},"agent_actions":{"view_html":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53","download_json":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53.json","view_paper":"https://pith.science/paper/V5QOQBWA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.11691&json=true","fetch_graph":"https://pith.science/api/pith-number/V5QOQBWAXPUYDWKQ55TM3W2P53/graph.json","fetch_events":"https://pith.science/api/pith-number/V5QOQBWAXPUYDWKQ55TM3W2P53/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53/action/storage_attestation","attest_author":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53/action/author_attestation","sign_citation":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53/action/citation_signature","submit_replication":"https://pith.science/pith/V5QOQBWAXPUYDWKQ55TM3W2P53/action/replication_record"}},"created_at":"2026-07-05T06:43:38.975142+00:00","updated_at":"2026-07-05T06:43:38.975142+00:00"}