{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:XFZDWTILS3BK6FHUKPBQLIG3OS","short_pith_number":"pith:XFZDWTIL","schema_version":"1.0","canonical_sha256":"b9723b4d0b96c2af14f453c305a0db74aa45e3e31e95057b883e982514cf0fce","source":{"kind":"arxiv","id":"1412.7428","version":1},"attestation_state":"computed","paper":{"title":"Spectroscopic Observations of a Coronal Loop: Basic Physical Plasma Parameters Along the Full Loop Length","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Durgesh Tripathi, G. R. Gupta, Helen E. Mason","submitted_at":"2014-12-23T16:17:22Z","abstract_excerpt":"Coronal loops are the basic structures of the solar transition region and corona. The understanding of physical mechanism behind the loop heating, plasma flows, and filling are still considered a major challenge in the solar physics. The mechanism(s) should be able to supply mass to the corona from the chromosphere and able to heat the plasma over 1 MK within the small distance of few hundred km from the chromosphere to the corona. This problem makes coronal loops an interesting target for detailed study. In this study, we focus on spectroscopic observations of a coronal loop, observed in its "},"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":"1412.7428","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-12-23T16:17:22Z","cross_cats_sorted":[],"title_canon_sha256":"dde482e670a05d262408fed63992ad1a6198bf27634a4a455a8c6625e7e2f0a1","abstract_canon_sha256":"cf2fc0a95b7e4780829211df109e32a448513ab7d70404a545969b9c068f19d1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:26:38.423777Z","signature_b64":"BlmqXy2g3YkSeAjQqBHCzyks+LhUz8EfqJSFcYvg/xSEkXf+75FLLvqjz+T3gJHVG3N4FOZk6ByBao+d+jsADw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b9723b4d0b96c2af14f453c305a0db74aa45e3e31e95057b883e982514cf0fce","last_reissued_at":"2026-05-18T02:26:38.423311Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:26:38.423311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectroscopic Observations of a Coronal Loop: Basic Physical Plasma Parameters Along the Full Loop Length","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Durgesh Tripathi, G. R. Gupta, Helen E. Mason","submitted_at":"2014-12-23T16:17:22Z","abstract_excerpt":"Coronal loops are the basic structures of the solar transition region and corona. The understanding of physical mechanism behind the loop heating, plasma flows, and filling are still considered a major challenge in the solar physics. The mechanism(s) should be able to supply mass to the corona from the chromosphere and able to heat the plasma over 1 MK within the small distance of few hundred km from the chromosphere to the corona. This problem makes coronal loops an interesting target for detailed study. In this study, we focus on spectroscopic observations of a coronal loop, observed in its "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.7428","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":"1412.7428","created_at":"2026-05-18T02:26:38.423413+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.7428v1","created_at":"2026-05-18T02:26:38.423413+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.7428","created_at":"2026-05-18T02:26:38.423413+00:00"},{"alias_kind":"pith_short_12","alias_value":"XFZDWTILS3BK","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"XFZDWTILS3BK6FHU","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"XFZDWTIL","created_at":"2026-05-18T12:28:57.508820+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/XFZDWTILS3BK6FHUKPBQLIG3OS","json":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS.json","graph_json":"https://pith.science/api/pith-number/XFZDWTILS3BK6FHUKPBQLIG3OS/graph.json","events_json":"https://pith.science/api/pith-number/XFZDWTILS3BK6FHUKPBQLIG3OS/events.json","paper":"https://pith.science/paper/XFZDWTIL"},"agent_actions":{"view_html":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS","download_json":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS.json","view_paper":"https://pith.science/paper/XFZDWTIL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.7428&json=true","fetch_graph":"https://pith.science/api/pith-number/XFZDWTILS3BK6FHUKPBQLIG3OS/graph.json","fetch_events":"https://pith.science/api/pith-number/XFZDWTILS3BK6FHUKPBQLIG3OS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS/action/storage_attestation","attest_author":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS/action/author_attestation","sign_citation":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS/action/citation_signature","submit_replication":"https://pith.science/pith/XFZDWTILS3BK6FHUKPBQLIG3OS/action/replication_record"}},"created_at":"2026-05-18T02:26:38.423413+00:00","updated_at":"2026-05-18T02:26:38.423413+00:00"}