{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:65ODDWMUTBJR5OCLXU4MOFOQVQ","short_pith_number":"pith:65ODDWMU","schema_version":"1.0","canonical_sha256":"f75c31d99498531eb84bbd38c715d0ac057803a92db22a9fa4ac8f088f61255f","source":{"kind":"arxiv","id":"1008.2938","version":1},"attestation_state":"computed","paper":{"title":"Formation and disruption of current filaments in a flow-driven turbulent magnetosphere","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":["cond-mat.stat-mech","nlin.CG","physics.flu-dyn","physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"Laura F. Morales, Paul Charbonneau, Vadim M. Uritsky, William W. Liu","submitted_at":"2010-08-17T17:30:51Z","abstract_excerpt":"Recent observations have established that the magnetosphere is a system of natural complexity. The co-existence of multi-scale structures such as auroral arcs, turbulent convective flows, and scale-free distributions of energy perturbations has lacked a unified explanation, although there is strong reason to believe that they all stem from a common base of physics. In this paper we show that a slow but turbulent convection leads to the formation of multi-scale current filaments reminiscent of auroral arcs. The process involves an interplay between random shuffling of field lines and dissipatio"},"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":"1008.2938","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"physics.plasm-ph","submitted_at":"2010-08-17T17:30:51Z","cross_cats_sorted":["cond-mat.stat-mech","nlin.CG","physics.flu-dyn","physics.space-ph"],"title_canon_sha256":"ff289737135a466c2259c68e55edc8bce058e95e74ac0d7dee43a894a6f16d3a","abstract_canon_sha256":"93c865295b86fa37a37b221f6cb9f979ac4e2530be0de94abec5238281add319"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:47.383685Z","signature_b64":"gcevgu3MFLzsf9Bv9oMtkNNa4AdOBo/YbUSIZVOMvMIqvRL1iWU0G7toiV7FPiy/hem5f7MzoK1Xm2MEKS9XBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f75c31d99498531eb84bbd38c715d0ac057803a92db22a9fa4ac8f088f61255f","last_reissued_at":"2026-05-18T02:05:47.383025Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:47.383025Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Formation and disruption of current filaments in a flow-driven turbulent magnetosphere","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":["cond-mat.stat-mech","nlin.CG","physics.flu-dyn","physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"Laura F. Morales, Paul Charbonneau, Vadim M. Uritsky, William W. Liu","submitted_at":"2010-08-17T17:30:51Z","abstract_excerpt":"Recent observations have established that the magnetosphere is a system of natural complexity. The co-existence of multi-scale structures such as auroral arcs, turbulent convective flows, and scale-free distributions of energy perturbations has lacked a unified explanation, although there is strong reason to believe that they all stem from a common base of physics. In this paper we show that a slow but turbulent convection leads to the formation of multi-scale current filaments reminiscent of auroral arcs. The process involves an interplay between random shuffling of field lines and dissipatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.2938","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":"1008.2938","created_at":"2026-05-18T02:05:47.383128+00:00"},{"alias_kind":"arxiv_version","alias_value":"1008.2938v1","created_at":"2026-05-18T02:05:47.383128+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.2938","created_at":"2026-05-18T02:05:47.383128+00:00"},{"alias_kind":"pith_short_12","alias_value":"65ODDWMUTBJR","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_16","alias_value":"65ODDWMUTBJR5OCL","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_8","alias_value":"65ODDWMU","created_at":"2026-05-18T12:26:04.259169+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/65ODDWMUTBJR5OCLXU4MOFOQVQ","json":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ.json","graph_json":"https://pith.science/api/pith-number/65ODDWMUTBJR5OCLXU4MOFOQVQ/graph.json","events_json":"https://pith.science/api/pith-number/65ODDWMUTBJR5OCLXU4MOFOQVQ/events.json","paper":"https://pith.science/paper/65ODDWMU"},"agent_actions":{"view_html":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ","download_json":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ.json","view_paper":"https://pith.science/paper/65ODDWMU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1008.2938&json=true","fetch_graph":"https://pith.science/api/pith-number/65ODDWMUTBJR5OCLXU4MOFOQVQ/graph.json","fetch_events":"https://pith.science/api/pith-number/65ODDWMUTBJR5OCLXU4MOFOQVQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ/action/storage_attestation","attest_author":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ/action/author_attestation","sign_citation":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ/action/citation_signature","submit_replication":"https://pith.science/pith/65ODDWMUTBJR5OCLXU4MOFOQVQ/action/replication_record"}},"created_at":"2026-05-18T02:05:47.383128+00:00","updated_at":"2026-05-18T02:05:47.383128+00:00"}