{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:BSFSUHBNSFL6DL4JJBONOKE6SH","short_pith_number":"pith:BSFSUHBN","schema_version":"1.0","canonical_sha256":"0c8b2a1c2d9157e1af89485cd7289e91e6c36c681fde26b3f81a9ab6a25bca3a","source":{"kind":"arxiv","id":"1607.01329","version":1},"attestation_state":"computed","paper":{"title":"Plasma sloshing in pulse-heated solar and stellar coronal loops","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Reale","submitted_at":"2016-07-05T17:02:27Z","abstract_excerpt":"There is evidence that coronal heating is highly intermittent, and flares are the high energy extreme. The properties of the heat pulses are difficult to constrain. Here hydrodynamic loop modeling shows that several large amplitude oscillations (~ 20% in density) are triggered in flare light curves if the duration of the heat pulse is shorter that the sound crossing time of the flaring loop. The reason is that the plasma has not enough time to reach pressure equilibrium during the heating and traveling pressure fronts develop. The period is a few minutes for typical solar coronal loops, dictat"},"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":"1607.01329","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-07-05T17:02:27Z","cross_cats_sorted":[],"title_canon_sha256":"527df39117f157a21570dfcb81140ca095670612748d18e374286e44208084f7","abstract_canon_sha256":"522f30927f2c98a2cdbb86746589c5568f6f63399e609a5e24357a127b08e71c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:01.889372Z","signature_b64":"6mAVbksMNkXRTrrQbG+3W/2FtJWgg7nrIF/7C6Ms5ih6E5giIgJYTc8pyiZOKFOClZnihBGWsBKu1BQFtILnAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c8b2a1c2d9157e1af89485cd7289e91e6c36c681fde26b3f81a9ab6a25bca3a","last_reissued_at":"2026-05-18T01:10:01.888789Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:01.888789Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Plasma sloshing in pulse-heated solar and stellar coronal loops","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Reale","submitted_at":"2016-07-05T17:02:27Z","abstract_excerpt":"There is evidence that coronal heating is highly intermittent, and flares are the high energy extreme. The properties of the heat pulses are difficult to constrain. Here hydrodynamic loop modeling shows that several large amplitude oscillations (~ 20% in density) are triggered in flare light curves if the duration of the heat pulse is shorter that the sound crossing time of the flaring loop. The reason is that the plasma has not enough time to reach pressure equilibrium during the heating and traveling pressure fronts develop. The period is a few minutes for typical solar coronal loops, dictat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.01329","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":"1607.01329","created_at":"2026-05-18T01:10:01.888878+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.01329v1","created_at":"2026-05-18T01:10:01.888878+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.01329","created_at":"2026-05-18T01:10:01.888878+00:00"},{"alias_kind":"pith_short_12","alias_value":"BSFSUHBNSFL6","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"BSFSUHBNSFL6DL4J","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"BSFSUHBN","created_at":"2026-05-18T12:30:07.202191+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/BSFSUHBNSFL6DL4JJBONOKE6SH","json":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH.json","graph_json":"https://pith.science/api/pith-number/BSFSUHBNSFL6DL4JJBONOKE6SH/graph.json","events_json":"https://pith.science/api/pith-number/BSFSUHBNSFL6DL4JJBONOKE6SH/events.json","paper":"https://pith.science/paper/BSFSUHBN"},"agent_actions":{"view_html":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH","download_json":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH.json","view_paper":"https://pith.science/paper/BSFSUHBN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.01329&json=true","fetch_graph":"https://pith.science/api/pith-number/BSFSUHBNSFL6DL4JJBONOKE6SH/graph.json","fetch_events":"https://pith.science/api/pith-number/BSFSUHBNSFL6DL4JJBONOKE6SH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH/action/storage_attestation","attest_author":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH/action/author_attestation","sign_citation":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH/action/citation_signature","submit_replication":"https://pith.science/pith/BSFSUHBNSFL6DL4JJBONOKE6SH/action/replication_record"}},"created_at":"2026-05-18T01:10:01.888878+00:00","updated_at":"2026-05-18T01:10:01.888878+00:00"}