{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:VIMLL3I5U6GG2MJMHOVUGFR7IH","short_pith_number":"pith:VIMLL3I5","schema_version":"1.0","canonical_sha256":"aa18b5ed1da78c6d312c3bab43163f41f0ae5708577488d45ab4e0475af1ed8e","source":{"kind":"arxiv","id":"1512.06980","version":1},"attestation_state":"computed","paper":{"title":"Cassini in situ observations of long-duration magnetic reconnection in Saturn's magnetotail","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Aikaterina Radioti, Andrew J. Coates, Andrew P. Walsh, Ariah Kidder, Caitriona M. Jackman, Christopher S. Arridge, Dan B. Reisenfeld, Gang-Kai Poh, James A. Slavin, Jonathan P. Eastwood, Laurent Lamy, Martin Volwerk, Michele K. Dougherty, Michelle F. Thomsen, Nick Sergis, Nicolas Andr\\'e, Philippe Zarka, Xianzhe Jia","submitted_at":"2015-12-22T08:35:43Z","abstract_excerpt":"Magnetic reconnection is a fundamental process in solar system and astrophysical plasmas, through which stored magnetic energy associated with current sheets is converted into thermal, kinetic and wave energy. Magnetic reconnection is also thought to be a key process involved in shedding internally produced plasma from the giant magnetospheres at Jupiter and Saturn through topological reconfiguration of the magnetic field. The region where magnetic fields reconnect is known as the diffusion region and in this letter we report on the first encounter of the Cassini spacecraft with a diffusion re"},"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":"1512.06980","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-12-22T08:35:43Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"9cf7eeda52a1d9c8a5d5f82a8328196265d853f84ebaa77cd76d0c98e036f461","abstract_canon_sha256":"5b3535f8772776091c9291e0e04937a96d994801b0b4a33148947795f54b6a3e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:53.247453Z","signature_b64":"Rt8/kei4eFw01JuKKP27Wbaj9V1pRHdsB8Lus44BbMEgVbHPBeWN29BtnBbhnuaQ4XABXmYZsJ1EV/e75wIYAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aa18b5ed1da78c6d312c3bab43163f41f0ae5708577488d45ab4e0475af1ed8e","last_reissued_at":"2026-05-18T01:23:53.246762Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:53.246762Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cassini in situ observations of long-duration magnetic reconnection in Saturn's magnetotail","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Aikaterina Radioti, Andrew J. Coates, Andrew P. Walsh, Ariah Kidder, Caitriona M. Jackman, Christopher S. Arridge, Dan B. Reisenfeld, Gang-Kai Poh, James A. Slavin, Jonathan P. Eastwood, Laurent Lamy, Martin Volwerk, Michele K. Dougherty, Michelle F. Thomsen, Nick Sergis, Nicolas Andr\\'e, Philippe Zarka, Xianzhe Jia","submitted_at":"2015-12-22T08:35:43Z","abstract_excerpt":"Magnetic reconnection is a fundamental process in solar system and astrophysical plasmas, through which stored magnetic energy associated with current sheets is converted into thermal, kinetic and wave energy. Magnetic reconnection is also thought to be a key process involved in shedding internally produced plasma from the giant magnetospheres at Jupiter and Saturn through topological reconfiguration of the magnetic field. The region where magnetic fields reconnect is known as the diffusion region and in this letter we report on the first encounter of the Cassini spacecraft with a diffusion re"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.06980","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":"1512.06980","created_at":"2026-05-18T01:23:53.246876+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.06980v1","created_at":"2026-05-18T01:23:53.246876+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.06980","created_at":"2026-05-18T01:23:53.246876+00:00"},{"alias_kind":"pith_short_12","alias_value":"VIMLL3I5U6GG","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_16","alias_value":"VIMLL3I5U6GG2MJM","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_8","alias_value":"VIMLL3I5","created_at":"2026-05-18T12:29:44.643036+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/VIMLL3I5U6GG2MJMHOVUGFR7IH","json":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH.json","graph_json":"https://pith.science/api/pith-number/VIMLL3I5U6GG2MJMHOVUGFR7IH/graph.json","events_json":"https://pith.science/api/pith-number/VIMLL3I5U6GG2MJMHOVUGFR7IH/events.json","paper":"https://pith.science/paper/VIMLL3I5"},"agent_actions":{"view_html":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH","download_json":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH.json","view_paper":"https://pith.science/paper/VIMLL3I5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.06980&json=true","fetch_graph":"https://pith.science/api/pith-number/VIMLL3I5U6GG2MJMHOVUGFR7IH/graph.json","fetch_events":"https://pith.science/api/pith-number/VIMLL3I5U6GG2MJMHOVUGFR7IH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH/action/storage_attestation","attest_author":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH/action/author_attestation","sign_citation":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH/action/citation_signature","submit_replication":"https://pith.science/pith/VIMLL3I5U6GG2MJMHOVUGFR7IH/action/replication_record"}},"created_at":"2026-05-18T01:23:53.246876+00:00","updated_at":"2026-05-18T01:23:53.246876+00:00"}