{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:TCCBBJL5E5ZAUIT7YB32FZNHQJ","short_pith_number":"pith:TCCBBJL5","schema_version":"1.0","canonical_sha256":"988410a57d27720a227fc077a2e5a78264cbb5678e2341daa9707fbe74d0ca37","source":{"kind":"arxiv","id":"2502.01796","version":1},"attestation_state":"computed","paper":{"title":"Coronal energy release by MHD avalanches III. Identification of a reconnection outflow from a nanoflare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Petralia, B. De Pontieu, F. Reale, G. Cozzo, J. Martinez-Sykora, P. Pagano, P. Testa, V. Hansteen","submitted_at":"2025-02-03T20:20:31Z","abstract_excerpt":"Outflows perpendicular to the guide field are believed to be a possible signature of magnetic reconnection in the solar corona and specifically a way to detect the occurrence of ubiquitous small-angle magnetic reconnection. The aim of this work is to identify possible diagnostic techniques of such outflows in hot coronal loops with SDO/AIA and the forthcoming MUltislit Solar Explorer (MUSE), in a realistically dynamic coronal loop environment in which an MHD avalanche is occurring. We consider a 3D MHD model of two magnetic flux tubes, including a stratified, radiative and thermal-conducting a"},"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":"2502.01796","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2025-02-03T20:20:31Z","cross_cats_sorted":[],"title_canon_sha256":"37083e755d75f76f081622bba9f0a61a7f66d7c06bb08f01befad793d8209f2f","abstract_canon_sha256":"6e19dab22f3a8947975a6ddd3e9f25d8a0a75f71448d7aad7332065a029a6f45"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:24:00.522240Z","signature_b64":"32XDnVEdE98u4MkKwMLjBSTuwDUiWbrutTTb3zZRi21wpcRJiSmTVuREbdydhZ3VHLMYoYsl7ViSFbPCxoL1Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"988410a57d27720a227fc077a2e5a78264cbb5678e2341daa9707fbe74d0ca37","last_reissued_at":"2026-07-05T10:24:00.521138Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:24:00.521138Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Coronal energy release by MHD avalanches III. Identification of a reconnection outflow from a nanoflare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Petralia, B. De Pontieu, F. Reale, G. Cozzo, J. Martinez-Sykora, P. Pagano, P. Testa, V. Hansteen","submitted_at":"2025-02-03T20:20:31Z","abstract_excerpt":"Outflows perpendicular to the guide field are believed to be a possible signature of magnetic reconnection in the solar corona and specifically a way to detect the occurrence of ubiquitous small-angle magnetic reconnection. The aim of this work is to identify possible diagnostic techniques of such outflows in hot coronal loops with SDO/AIA and the forthcoming MUltislit Solar Explorer (MUSE), in a realistically dynamic coronal loop environment in which an MHD avalanche is occurring. We consider a 3D MHD model of two magnetic flux tubes, including a stratified, radiative and thermal-conducting a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.01796","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2502.01796/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2502.01796","created_at":"2026-07-05T10:24:00.521336+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.01796v1","created_at":"2026-07-05T10:24:00.521336+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.01796","created_at":"2026-07-05T10:24:00.521336+00:00"},{"alias_kind":"pith_short_12","alias_value":"TCCBBJL5E5ZA","created_at":"2026-07-05T10:24:00.521336+00:00"},{"alias_kind":"pith_short_16","alias_value":"TCCBBJL5E5ZAUIT7","created_at":"2026-07-05T10:24:00.521336+00:00"},{"alias_kind":"pith_short_8","alias_value":"TCCBBJL5","created_at":"2026-07-05T10:24:00.521336+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.13981","citing_title":"Deciphering the Formation and Dynamics of Double-decker Filament Through Component Magnetic Reconnection","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ","json":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ.json","graph_json":"https://pith.science/api/pith-number/TCCBBJL5E5ZAUIT7YB32FZNHQJ/graph.json","events_json":"https://pith.science/api/pith-number/TCCBBJL5E5ZAUIT7YB32FZNHQJ/events.json","paper":"https://pith.science/paper/TCCBBJL5"},"agent_actions":{"view_html":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ","download_json":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ.json","view_paper":"https://pith.science/paper/TCCBBJL5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.01796&json=true","fetch_graph":"https://pith.science/api/pith-number/TCCBBJL5E5ZAUIT7YB32FZNHQJ/graph.json","fetch_events":"https://pith.science/api/pith-number/TCCBBJL5E5ZAUIT7YB32FZNHQJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ/action/storage_attestation","attest_author":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ/action/author_attestation","sign_citation":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ/action/citation_signature","submit_replication":"https://pith.science/pith/TCCBBJL5E5ZAUIT7YB32FZNHQJ/action/replication_record"}},"created_at":"2026-07-05T10:24:00.521336+00:00","updated_at":"2026-07-05T10:24:00.521336+00:00"}