{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:SJRJ3W3ALMNTTVV5BPQ3WJ66KR","short_pith_number":"pith:SJRJ3W3A","schema_version":"1.0","canonical_sha256":"92629ddb605b1b39d6bd0be1bb27de5471f060cd43f3f311609d3739607c8262","source":{"kind":"arxiv","id":"1605.06343","version":2},"attestation_state":"computed","paper":{"title":"Particle Acceleration in Collapsing Magnetic Traps with a Braking Plasma Jet","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Alexei Borissov, James Threlfall, Thomas Neukirch","submitted_at":"2016-05-20T13:15:33Z","abstract_excerpt":"Collapsing magnetic traps (CMTs) are one proposed mechanism for generating non-thermal particle populations in solar flares. CMTs occur if an initially stretched magnetic field structure relaxes rapidly into a lower-energy configuration, which is believed to happen as a by-product of magnetic reconnection. A similar mechanism for energising particles has also been found to operate in the Earth's magnetotail. One particular feature proposed to be of importance for particle acceleration in the magnetotail is that of a braking plasma jet, i.e. a localised region of strong flow encountering strong"},"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":"1605.06343","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-05-20T13:15:33Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"6c48487dbb89f9acdce23bf018367982fc322790cd731fa4a3618838e257e893","abstract_canon_sha256":"1855bdd29b7b24d1a93f1e2397af92efb0145c6b6c0bff337da2de0f7b57e5b0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:19.785166Z","signature_b64":"K7GPl1WKo/GIlQDLDGNooCy6iTCAZ+7O63tVKnH9GUKiYSwSrHYdQ/CjkcrmGiFU1ZbDj6nSjgJksxS66wsmBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"92629ddb605b1b39d6bd0be1bb27de5471f060cd43f3f311609d3739607c8262","last_reissued_at":"2026-05-18T01:10:19.784741Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:19.784741Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Particle Acceleration in Collapsing Magnetic Traps with a Braking Plasma Jet","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Alexei Borissov, James Threlfall, Thomas Neukirch","submitted_at":"2016-05-20T13:15:33Z","abstract_excerpt":"Collapsing magnetic traps (CMTs) are one proposed mechanism for generating non-thermal particle populations in solar flares. CMTs occur if an initially stretched magnetic field structure relaxes rapidly into a lower-energy configuration, which is believed to happen as a by-product of magnetic reconnection. A similar mechanism for energising particles has also been found to operate in the Earth's magnetotail. One particular feature proposed to be of importance for particle acceleration in the magnetotail is that of a braking plasma jet, i.e. a localised region of strong flow encountering strong"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.06343","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":"1605.06343","created_at":"2026-05-18T01:10:19.784806+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.06343v2","created_at":"2026-05-18T01:10:19.784806+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.06343","created_at":"2026-05-18T01:10:19.784806+00:00"},{"alias_kind":"pith_short_12","alias_value":"SJRJ3W3ALMNT","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"SJRJ3W3ALMNTTVV5","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"SJRJ3W3A","created_at":"2026-05-18T12:30:44.179134+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.04293","citing_title":"Transport of electrons in tangled magnetic fields","ref_index":47,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR","json":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR.json","graph_json":"https://pith.science/api/pith-number/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/graph.json","events_json":"https://pith.science/api/pith-number/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/events.json","paper":"https://pith.science/paper/SJRJ3W3A"},"agent_actions":{"view_html":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR","download_json":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR.json","view_paper":"https://pith.science/paper/SJRJ3W3A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.06343&json=true","fetch_graph":"https://pith.science/api/pith-number/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/graph.json","fetch_events":"https://pith.science/api/pith-number/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/action/storage_attestation","attest_author":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/action/author_attestation","sign_citation":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/action/citation_signature","submit_replication":"https://pith.science/pith/SJRJ3W3ALMNTTVV5BPQ3WJ66KR/action/replication_record"}},"created_at":"2026-05-18T01:10:19.784806+00:00","updated_at":"2026-05-18T01:10:19.784806+00:00"}