{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:JMYXE7KBU6DSJG2OGCKPUYR7CZ","short_pith_number":"pith:JMYXE7KB","schema_version":"1.0","canonical_sha256":"4b31727d41a787249b4e3094fa623f1665f83912d70ccc0d962ab45892243d9e","source":{"kind":"arxiv","id":"1405.0130","version":2},"attestation_state":"computed","paper":{"title":"Energy Loss of Solar $p$ Modes due to the excitation of Magnetic Sausage Tube Waves: Importance of Coupling the Upper Atmosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrew Gascoyne, Bradley Hindman, Rekha Jain","submitted_at":"2014-05-01T10:47:51Z","abstract_excerpt":"We consider damping and absorption of solar $p$ modes due to their energy loss to magnetic tube waves that can freely carry energy out of the acoustic cavity. The coupling of $p$ modes and sausage tube waves is studied in a model atmosphere composed of a polytropic interior above which lies an isothermal upper atmosphere. The sausage tube waves, excited by $p$ modes, propagate along a magnetic fibril which is assumed to be a vertically aligned, stratified, thin magnetic flux-tube. The deficit of $p$-mode energy is quantified through the damping rate, $\\Gamma$ and absorption coefficient, $\\alph"},"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":"1405.0130","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-05-01T10:47:51Z","cross_cats_sorted":[],"title_canon_sha256":"98e86ae8db298065e518b12b78d6b26644305c896d9e3a6a607c46ae48907b83","abstract_canon_sha256":"6eb8188600ee282341719a7f31b0a9cf6bebb80d7c2d3786fa540c6a89f00ebe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:21.092258Z","signature_b64":"643NSK5uNrS+nbY27+zpWIzvgXS8ws5UeXDL4i2s18MGmaXfrghF34rZ4PTN05ji1iWD28bSkjqHMfToT5CWBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4b31727d41a787249b4e3094fa623f1665f83912d70ccc0d962ab45892243d9e","last_reissued_at":"2026-05-18T01:43:21.091562Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:21.091562Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Energy Loss of Solar $p$ Modes due to the excitation of Magnetic Sausage Tube Waves: Importance of Coupling the Upper Atmosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrew Gascoyne, Bradley Hindman, Rekha Jain","submitted_at":"2014-05-01T10:47:51Z","abstract_excerpt":"We consider damping and absorption of solar $p$ modes due to their energy loss to magnetic tube waves that can freely carry energy out of the acoustic cavity. The coupling of $p$ modes and sausage tube waves is studied in a model atmosphere composed of a polytropic interior above which lies an isothermal upper atmosphere. The sausage tube waves, excited by $p$ modes, propagate along a magnetic fibril which is assumed to be a vertically aligned, stratified, thin magnetic flux-tube. The deficit of $p$-mode energy is quantified through the damping rate, $\\Gamma$ and absorption coefficient, $\\alph"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.0130","kind":"arxiv","version":2},"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":"1405.0130","created_at":"2026-05-18T01:43:21.091695+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.0130v2","created_at":"2026-05-18T01:43:21.091695+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.0130","created_at":"2026-05-18T01:43:21.091695+00:00"},{"alias_kind":"pith_short_12","alias_value":"JMYXE7KBU6DS","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_16","alias_value":"JMYXE7KBU6DSJG2O","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_8","alias_value":"JMYXE7KB","created_at":"2026-05-18T12:28:33.132498+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/JMYXE7KBU6DSJG2OGCKPUYR7CZ","json":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ.json","graph_json":"https://pith.science/api/pith-number/JMYXE7KBU6DSJG2OGCKPUYR7CZ/graph.json","events_json":"https://pith.science/api/pith-number/JMYXE7KBU6DSJG2OGCKPUYR7CZ/events.json","paper":"https://pith.science/paper/JMYXE7KB"},"agent_actions":{"view_html":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ","download_json":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ.json","view_paper":"https://pith.science/paper/JMYXE7KB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.0130&json=true","fetch_graph":"https://pith.science/api/pith-number/JMYXE7KBU6DSJG2OGCKPUYR7CZ/graph.json","fetch_events":"https://pith.science/api/pith-number/JMYXE7KBU6DSJG2OGCKPUYR7CZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ/action/storage_attestation","attest_author":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ/action/author_attestation","sign_citation":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ/action/citation_signature","submit_replication":"https://pith.science/pith/JMYXE7KBU6DSJG2OGCKPUYR7CZ/action/replication_record"}},"created_at":"2026-05-18T01:43:21.091695+00:00","updated_at":"2026-05-18T01:43:21.091695+00:00"}