{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:HHP553VMO6HNJWCNA7CGHMY4PH","short_pith_number":"pith:HHP553VM","schema_version":"1.0","canonical_sha256":"39dfdeeeac778ed4d84d07c463b31c79fbd47e93a783ff517956bc66d0b8d85f","source":{"kind":"arxiv","id":"1411.7465","version":1},"attestation_state":"computed","paper":{"title":"New analytical and numerical models of solar coronal loop: I. Application to forced vertical kink oscillations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A.K. Srivastava, A. Solov'ev, J. Kraskiewicz, K. Murawski","submitted_at":"2014-11-27T04:07:42Z","abstract_excerpt":"Aims. We construct a new analytical model of a solar coronal loop that is embedded in a gravitationally stratified and magnetically confined atmosphere. On the basis of this analytical model, we devise a numerical model of solar coronal loops. We adopt it to perform the numerical simulations of its vertical kink oscillations excited by an external driver. Methods. Our model of the solar atmosphere is constructed by adopting a realistic temperature distribution and specifying the curved magnetic field lines that constitute a coronal loop. This loop is described by 2D, ideal magnetohydro- dynami"},"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":"1411.7465","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-11-27T04:07:42Z","cross_cats_sorted":[],"title_canon_sha256":"fd67e192dac1cedf943025d79ec6f1175e32c792cf6cf36e2d484b183fe322ea","abstract_canon_sha256":"f38e7934154173a2540c9c32d6e13803e9ff6c2cfa228dba8e749ac69956a1c0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:20:30.492383Z","signature_b64":"kSc/YrI8wP8hJdW+2DHWxFPXNkDsa4TXNzMis139YRk4UCQu5t3jm8eQpQIj7msOyfU3ix8IqNJ9dydPpCdEAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"39dfdeeeac778ed4d84d07c463b31c79fbd47e93a783ff517956bc66d0b8d85f","last_reissued_at":"2026-05-18T02:20:30.491806Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:20:30.491806Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New analytical and numerical models of solar coronal loop: I. Application to forced vertical kink oscillations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A.K. Srivastava, A. Solov'ev, J. Kraskiewicz, K. Murawski","submitted_at":"2014-11-27T04:07:42Z","abstract_excerpt":"Aims. We construct a new analytical model of a solar coronal loop that is embedded in a gravitationally stratified and magnetically confined atmosphere. On the basis of this analytical model, we devise a numerical model of solar coronal loops. We adopt it to perform the numerical simulations of its vertical kink oscillations excited by an external driver. Methods. Our model of the solar atmosphere is constructed by adopting a realistic temperature distribution and specifying the curved magnetic field lines that constitute a coronal loop. This loop is described by 2D, ideal magnetohydro- dynami"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.7465","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":"1411.7465","created_at":"2026-05-18T02:20:30.491892+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.7465v1","created_at":"2026-05-18T02:20:30.491892+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.7465","created_at":"2026-05-18T02:20:30.491892+00:00"},{"alias_kind":"pith_short_12","alias_value":"HHP553VMO6HN","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_16","alias_value":"HHP553VMO6HNJWCN","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_8","alias_value":"HHP553VM","created_at":"2026-05-18T12:28:30.664211+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/HHP553VMO6HNJWCNA7CGHMY4PH","json":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH.json","graph_json":"https://pith.science/api/pith-number/HHP553VMO6HNJWCNA7CGHMY4PH/graph.json","events_json":"https://pith.science/api/pith-number/HHP553VMO6HNJWCNA7CGHMY4PH/events.json","paper":"https://pith.science/paper/HHP553VM"},"agent_actions":{"view_html":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH","download_json":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH.json","view_paper":"https://pith.science/paper/HHP553VM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.7465&json=true","fetch_graph":"https://pith.science/api/pith-number/HHP553VMO6HNJWCNA7CGHMY4PH/graph.json","fetch_events":"https://pith.science/api/pith-number/HHP553VMO6HNJWCNA7CGHMY4PH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH/action/storage_attestation","attest_author":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH/action/author_attestation","sign_citation":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH/action/citation_signature","submit_replication":"https://pith.science/pith/HHP553VMO6HNJWCNA7CGHMY4PH/action/replication_record"}},"created_at":"2026-05-18T02:20:30.491892+00:00","updated_at":"2026-05-18T02:20:30.491892+00:00"}