{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:BWQ2ZZ2FK6BJMADUL3F6BGTHJW","short_pith_number":"pith:BWQ2ZZ2F","schema_version":"1.0","canonical_sha256":"0da1ace74557829600745ecbe09a674d918c1cc4a56bd998d46662f85023e20d","source":{"kind":"arxiv","id":"1610.04732","version":1},"attestation_state":"computed","paper":{"title":"Anomalous Cooling of Coronal Loops with Turbulent Suppression of Thermal Conduction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Gordon Emslie, Eduard P. Kontar, Jonathan M. Watters, Nicolas H. Bian","submitted_at":"2016-10-15T13:29:32Z","abstract_excerpt":"We investigate the impact of turbulent suppression of parallel heat conduction on the cooling of post-flare coronal loops. Depending on the value of the mean free path $\\lambda_T$ associated with the turbulent scattering process, we identify four main cooling scenarios. The overall temperature evolution, from an initial temperature in excess of $10^7$~K, is modeled in each case, highlighting the evolution of the dominant cooling mechanism throughout the cooling process. Comparison with observed cooling times allows the value of $\\lambda_T$ to be constrained, and interestingly this range corres"},"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":"1610.04732","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-15T13:29:32Z","cross_cats_sorted":[],"title_canon_sha256":"271d146d7cd9e5b882e7097b47d3262e118543193aa78da17645b57d5a40fcbf","abstract_canon_sha256":"3f8027cdefba3dd3346c9340997c60094625dd81516122fe38fa0cea027f218d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:55:07.049127Z","signature_b64":"a/TE9nhLzNOWycRkcbJYq8TQqWlXP8R4GNO09/Wb71TJyvNwioN8adiHHWybh9ScApZOEGndy+lEs5TWMuujAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0da1ace74557829600745ecbe09a674d918c1cc4a56bd998d46662f85023e20d","last_reissued_at":"2026-05-18T00:55:07.048498Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:55:07.048498Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Anomalous Cooling of Coronal Loops with Turbulent Suppression of Thermal Conduction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Gordon Emslie, Eduard P. Kontar, Jonathan M. Watters, Nicolas H. Bian","submitted_at":"2016-10-15T13:29:32Z","abstract_excerpt":"We investigate the impact of turbulent suppression of parallel heat conduction on the cooling of post-flare coronal loops. Depending on the value of the mean free path $\\lambda_T$ associated with the turbulent scattering process, we identify four main cooling scenarios. The overall temperature evolution, from an initial temperature in excess of $10^7$~K, is modeled in each case, highlighting the evolution of the dominant cooling mechanism throughout the cooling process. Comparison with observed cooling times allows the value of $\\lambda_T$ to be constrained, and interestingly this range corres"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.04732","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":"1610.04732","created_at":"2026-05-18T00:55:07.048585+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.04732v1","created_at":"2026-05-18T00:55:07.048585+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.04732","created_at":"2026-05-18T00:55:07.048585+00:00"},{"alias_kind":"pith_short_12","alias_value":"BWQ2ZZ2FK6BJ","created_at":"2026-05-18T12:30:09.641336+00:00"},{"alias_kind":"pith_short_16","alias_value":"BWQ2ZZ2FK6BJMADU","created_at":"2026-05-18T12:30:09.641336+00:00"},{"alias_kind":"pith_short_8","alias_value":"BWQ2ZZ2F","created_at":"2026-05-18T12:30:09.641336+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/BWQ2ZZ2FK6BJMADUL3F6BGTHJW","json":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW.json","graph_json":"https://pith.science/api/pith-number/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/graph.json","events_json":"https://pith.science/api/pith-number/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/events.json","paper":"https://pith.science/paper/BWQ2ZZ2F"},"agent_actions":{"view_html":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW","download_json":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW.json","view_paper":"https://pith.science/paper/BWQ2ZZ2F","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.04732&json=true","fetch_graph":"https://pith.science/api/pith-number/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/graph.json","fetch_events":"https://pith.science/api/pith-number/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/action/storage_attestation","attest_author":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/action/author_attestation","sign_citation":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/action/citation_signature","submit_replication":"https://pith.science/pith/BWQ2ZZ2FK6BJMADUL3F6BGTHJW/action/replication_record"}},"created_at":"2026-05-18T00:55:07.048585+00:00","updated_at":"2026-05-18T00:55:07.048585+00:00"}