{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:5QAVMEY7ZQ6FLVASQQNZNDW5WC","short_pith_number":"pith:5QAVMEY7","schema_version":"1.0","canonical_sha256":"ec0156131fcc3c55d412841b968eddb08cdba66a198f76858a5e064843c08874","source":{"kind":"arxiv","id":"astro-ph/0107138","version":1},"attestation_state":"computed","paper":{"title":"Source Regions of Coronal Mass Ejections","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) Naval Research Lab, DC, India, K. P. Dere (2) ((1) IUCAA, Prasad Subramanian (1), Pune, USA), Washington","submitted_at":"2001-07-07T09:15:53Z","abstract_excerpt":"Observations of the solar corona with the Large Angle Spectrometric Coronograph (LASCO) and Extreme ultraviolet Imaging Telescope (EIT) instruments on the Solar and Heliospheric Observatory (SOHO) provide an unprecedented opportunity to study coronal mass ejections (CMEs) from their initiation through their evolution out to 30 \\rsun. The objective of this study is to gain an understanding of the source regions from which the CMEs emanate. To this end, we have developed a list of 32 CMEs whose source regions are located on the solar disk and are well observed in EIT 195 {\\AA} data during the pe"},"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":"astro-ph/0107138","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-07-07T09:15:53Z","cross_cats_sorted":[],"title_canon_sha256":"88adc87a54f6f845b49f0fe43a2ec8ce7b25691a85ba38d033157c0dce9945ff","abstract_canon_sha256":"8022e99a24014ccd1077d061b71c55d10488044597a0f84814a482589187674b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:23:40.422120Z","signature_b64":"lsmYZgyM8+IpQhYMEyvOP/1TnLz+d8rWOSU64QkgzpDdzOJwWMMg1mwIzeXRTs78t8RaqJV9T8YqGoDR9v0qDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ec0156131fcc3c55d412841b968eddb08cdba66a198f76858a5e064843c08874","last_reissued_at":"2026-07-04T16:23:40.421681Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:23:40.421681Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Source Regions of Coronal Mass Ejections","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) Naval Research Lab, DC, India, K. P. Dere (2) ((1) IUCAA, Prasad Subramanian (1), Pune, USA), Washington","submitted_at":"2001-07-07T09:15:53Z","abstract_excerpt":"Observations of the solar corona with the Large Angle Spectrometric Coronograph (LASCO) and Extreme ultraviolet Imaging Telescope (EIT) instruments on the Solar and Heliospheric Observatory (SOHO) provide an unprecedented opportunity to study coronal mass ejections (CMEs) from their initiation through their evolution out to 30 \\rsun. The objective of this study is to gain an understanding of the source regions from which the CMEs emanate. To this end, we have developed a list of 32 CMEs whose source regions are located on the solar disk and are well observed in EIT 195 {\\AA} data during the pe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0107138","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/astro-ph/0107138/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":"astro-ph/0107138","created_at":"2026-07-04T16:23:40.421738+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0107138v1","created_at":"2026-07-04T16:23:40.421738+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0107138","created_at":"2026-07-04T16:23:40.421738+00:00"},{"alias_kind":"pith_short_12","alias_value":"5QAVMEY7ZQ6F","created_at":"2026-07-04T16:23:40.421738+00:00"},{"alias_kind":"pith_short_16","alias_value":"5QAVMEY7ZQ6FLVAS","created_at":"2026-07-04T16:23:40.421738+00:00"},{"alias_kind":"pith_short_8","alias_value":"5QAVMEY7","created_at":"2026-07-04T16:23:40.421738+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.04196","citing_title":"Probing Flare-Associated Eruptions on AB Doradus via X-ray Absorption Variations","ref_index":53,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC","json":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC.json","graph_json":"https://pith.science/api/pith-number/5QAVMEY7ZQ6FLVASQQNZNDW5WC/graph.json","events_json":"https://pith.science/api/pith-number/5QAVMEY7ZQ6FLVASQQNZNDW5WC/events.json","paper":"https://pith.science/paper/5QAVMEY7"},"agent_actions":{"view_html":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC","download_json":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC.json","view_paper":"https://pith.science/paper/5QAVMEY7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0107138&json=true","fetch_graph":"https://pith.science/api/pith-number/5QAVMEY7ZQ6FLVASQQNZNDW5WC/graph.json","fetch_events":"https://pith.science/api/pith-number/5QAVMEY7ZQ6FLVASQQNZNDW5WC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC/action/storage_attestation","attest_author":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC/action/author_attestation","sign_citation":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC/action/citation_signature","submit_replication":"https://pith.science/pith/5QAVMEY7ZQ6FLVASQQNZNDW5WC/action/replication_record"}},"created_at":"2026-07-04T16:23:40.421738+00:00","updated_at":"2026-07-04T16:23:40.421738+00:00"}