{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:AFWVA3TPYKB4RYFKSM75JVT6GK","short_pith_number":"pith:AFWVA3TP","schema_version":"1.0","canonical_sha256":"016d506e6fc283c8e0aa933fd4d67e32ba4f795c0a928ca8f53c642ed444a9dd","source":{"kind":"arxiv","id":"2505.19228","version":1},"attestation_state":"computed","paper":{"title":"Coronal dimmings and what they tell us about solar and stellar coronal mass ejections","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Angelos Vourlidas, Astrid M. Veronig, Avijeet Prasad, Barbara Thompson, Bernhard Kliem, Cooper Downs, Hugh S. Hudson, Hui Tian, Jiong Qiu, Karin Dissauer, Meng Jin, Rachel Osten, Tatiana Podladchikova","submitted_at":"2025-05-25T16:44:19Z","abstract_excerpt":"Coronal dimmings associated with coronal mass ejections (CME) from the Sun have gained much attention since the late 1990s when they were first observed in high-cadence imagery of the SOHO/EIT and Yohkoh/SXT instruments. They appear as localized sudden decreases of the coronal emission at extreme ultraviolet (EUV) and soft X-ray (SXR) wavelengths, that evolve impulsively during the lift-off and early expansion phase of a CME. Coronal dimmings have been interpreted as \"footprints\" of the erupting flux rope and also as indicators of the coronal mass loss by CMEs. However, these are only some asp"},"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":"2505.19228","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2025-05-25T16:44:19Z","cross_cats_sorted":[],"title_canon_sha256":"8703d6039dd10ff014339a3d353fcf5edbddfccfe78d8f7a6e704b3c4d2d2122","abstract_canon_sha256":"95ef20a67c1e24dac730925c8363d6bdc5b92a519c06e4790d438285612fa1c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:09:26.792214Z","signature_b64":"P3Cn2lELwlWsfj0nhH3Exx6FMxKb7Y68lYDHIrxCHqA2s5f4TqeFM5lOHbhripK7nKhxt7GZX7G75U+CTRpWCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"016d506e6fc283c8e0aa933fd4d67e32ba4f795c0a928ca8f53c642ed444a9dd","last_reissued_at":"2026-07-05T11:09:26.791722Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:09:26.791722Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Coronal dimmings and what they tell us about solar and stellar coronal mass ejections","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Angelos Vourlidas, Astrid M. Veronig, Avijeet Prasad, Barbara Thompson, Bernhard Kliem, Cooper Downs, Hugh S. Hudson, Hui Tian, Jiong Qiu, Karin Dissauer, Meng Jin, Rachel Osten, Tatiana Podladchikova","submitted_at":"2025-05-25T16:44:19Z","abstract_excerpt":"Coronal dimmings associated with coronal mass ejections (CME) from the Sun have gained much attention since the late 1990s when they were first observed in high-cadence imagery of the SOHO/EIT and Yohkoh/SXT instruments. They appear as localized sudden decreases of the coronal emission at extreme ultraviolet (EUV) and soft X-ray (SXR) wavelengths, that evolve impulsively during the lift-off and early expansion phase of a CME. Coronal dimmings have been interpreted as \"footprints\" of the erupting flux rope and also as indicators of the coronal mass loss by CMEs. However, these are only some asp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.19228","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/2505.19228/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":"2505.19228","created_at":"2026-07-05T11:09:26.791785+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.19228v1","created_at":"2026-07-05T11:09:26.791785+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.19228","created_at":"2026-07-05T11:09:26.791785+00:00"},{"alias_kind":"pith_short_12","alias_value":"AFWVA3TPYKB4","created_at":"2026-07-05T11:09:26.791785+00:00"},{"alias_kind":"pith_short_16","alias_value":"AFWVA3TPYKB4RYFK","created_at":"2026-07-05T11:09:26.791785+00:00"},{"alias_kind":"pith_short_8","alias_value":"AFWVA3TP","created_at":"2026-07-05T11:09:26.791785+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.22399","citing_title":"Reconstruction of annual solar irradiance over the last three millennia","ref_index":185,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK","json":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK.json","graph_json":"https://pith.science/api/pith-number/AFWVA3TPYKB4RYFKSM75JVT6GK/graph.json","events_json":"https://pith.science/api/pith-number/AFWVA3TPYKB4RYFKSM75JVT6GK/events.json","paper":"https://pith.science/paper/AFWVA3TP"},"agent_actions":{"view_html":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK","download_json":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK.json","view_paper":"https://pith.science/paper/AFWVA3TP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.19228&json=true","fetch_graph":"https://pith.science/api/pith-number/AFWVA3TPYKB4RYFKSM75JVT6GK/graph.json","fetch_events":"https://pith.science/api/pith-number/AFWVA3TPYKB4RYFKSM75JVT6GK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK/action/storage_attestation","attest_author":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK/action/author_attestation","sign_citation":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK/action/citation_signature","submit_replication":"https://pith.science/pith/AFWVA3TPYKB4RYFKSM75JVT6GK/action/replication_record"}},"created_at":"2026-07-05T11:09:26.791785+00:00","updated_at":"2026-07-05T11:09:26.791785+00:00"}