{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:7TWL75UTZGYQOUX67LBMSHO7FN","short_pith_number":"pith:7TWL75UT","schema_version":"1.0","canonical_sha256":"fcecbff693c9b10752fefac2c91ddf2b523aa9af0397ad780a1f36d53e87669d","source":{"kind":"arxiv","id":"1409.0458","version":1},"attestation_state":"computed","paper":{"title":"A Space Weather Mission Concept: Observatories of the Solar Corona and Active Regions (OSCAR)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Alankrita Isha Mrigakshi, Antoine Strugarek, Arrow Lee, Bernhard Seifert, Christoffer Stausland, Emil Kraaikamp, G\\\"unter Kargl, Liam O'Halloran, Malte Br\\\"ose, Nils Janitzek, Philippe Escoubet, Philipp L\\\"oschl, Sanni Hoilijoki, Sheila Spina, Sonny Massahi, Thomas Philippe, Victor Pereira Blanco","submitted_at":"2014-09-01T15:51:58Z","abstract_excerpt":"Coronal Mass Ejections (CMEs) and Corotating Interaction Regions (CIRs) are major sources of magnetic storms on Earth and are therefore considered to be the most dangerous space weather events. The Observatories of Solar Corona and Active Regions (OSCAR) mission is designed to identify the 3D structure of coronal loops and to study the trigger mechanisms of CMEs in solar Active Regions (ARs) as well as their evolution and propagation processes in the inner heliosphere. It also aims to provide monitoring and forecasting of geo-effective CMEs and CIRs. OSCAR would contribute to significant advan"},"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":"1409.0458","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-09-01T15:51:58Z","cross_cats_sorted":["astro-ph.IM","physics.space-ph"],"title_canon_sha256":"75947c3c3a1ed2e6d0e3d6e3e62dc9fd42c22835abc82f6c06a9f25b4e5fd1e3","abstract_canon_sha256":"ae91482084e4cff2027529a81657579aeb0634a10d5592239a1acaa3562095e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:43:52.728281Z","signature_b64":"uEs3WirzEORQgkMAKqwbGb0ohFQVeI6JgIkyNm6Mi1hJ8k5HkDOqgcM2Oz4R6myBiBxx5lipp9DP0Fg3/5qGCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fcecbff693c9b10752fefac2c91ddf2b523aa9af0397ad780a1f36d53e87669d","last_reissued_at":"2026-05-18T02:43:52.727783Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:43:52.727783Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Space Weather Mission Concept: Observatories of the Solar Corona and Active Regions (OSCAR)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Alankrita Isha Mrigakshi, Antoine Strugarek, Arrow Lee, Bernhard Seifert, Christoffer Stausland, Emil Kraaikamp, G\\\"unter Kargl, Liam O'Halloran, Malte Br\\\"ose, Nils Janitzek, Philippe Escoubet, Philipp L\\\"oschl, Sanni Hoilijoki, Sheila Spina, Sonny Massahi, Thomas Philippe, Victor Pereira Blanco","submitted_at":"2014-09-01T15:51:58Z","abstract_excerpt":"Coronal Mass Ejections (CMEs) and Corotating Interaction Regions (CIRs) are major sources of magnetic storms on Earth and are therefore considered to be the most dangerous space weather events. The Observatories of Solar Corona and Active Regions (OSCAR) mission is designed to identify the 3D structure of coronal loops and to study the trigger mechanisms of CMEs in solar Active Regions (ARs) as well as their evolution and propagation processes in the inner heliosphere. It also aims to provide monitoring and forecasting of geo-effective CMEs and CIRs. OSCAR would contribute to significant advan"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.0458","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":"1409.0458","created_at":"2026-05-18T02:43:52.727838+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.0458v1","created_at":"2026-05-18T02:43:52.727838+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.0458","created_at":"2026-05-18T02:43:52.727838+00:00"},{"alias_kind":"pith_short_12","alias_value":"7TWL75UTZGYQ","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_16","alias_value":"7TWL75UTZGYQOUX6","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_8","alias_value":"7TWL75UT","created_at":"2026-05-18T12:28:19.803747+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/7TWL75UTZGYQOUX67LBMSHO7FN","json":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN.json","graph_json":"https://pith.science/api/pith-number/7TWL75UTZGYQOUX67LBMSHO7FN/graph.json","events_json":"https://pith.science/api/pith-number/7TWL75UTZGYQOUX67LBMSHO7FN/events.json","paper":"https://pith.science/paper/7TWL75UT"},"agent_actions":{"view_html":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN","download_json":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN.json","view_paper":"https://pith.science/paper/7TWL75UT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.0458&json=true","fetch_graph":"https://pith.science/api/pith-number/7TWL75UTZGYQOUX67LBMSHO7FN/graph.json","fetch_events":"https://pith.science/api/pith-number/7TWL75UTZGYQOUX67LBMSHO7FN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN/action/storage_attestation","attest_author":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN/action/author_attestation","sign_citation":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN/action/citation_signature","submit_replication":"https://pith.science/pith/7TWL75UTZGYQOUX67LBMSHO7FN/action/replication_record"}},"created_at":"2026-05-18T02:43:52.727838+00:00","updated_at":"2026-05-18T02:43:52.727838+00:00"}