{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:TVB5UTNDJVHONOIT7E5PMIW43N","short_pith_number":"pith:TVB5UTND","schema_version":"1.0","canonical_sha256":"9d43da4da34d4ee6b913f93af622dcdb6b2a7cdecfe53474a4145daeec222785","source":{"kind":"arxiv","id":"1108.2138","version":2},"attestation_state":"computed","paper":{"title":"Toward a Realistic Pulsar Magnetosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"Alice Harding, Constantinos Kalapotharakos, Demosthenes Kazanas, Ioannis Contopoulos","submitted_at":"2011-08-10T10:16:43Z","abstract_excerpt":"We present the magnetic and electric field structures as well as the currents and charge densities of pulsar magnetospheres which do not obey the ideal condition, ${\\bf E \\cdot B =0}$. Since the acceleration of particles and the production of radiation requires the presence of an electric field component parallel to the magnetic field, ${\\bf E}_\\parallel$, the structure of non-Ideal pulsar magnetospheres is intimately related to the production of pulsar radiation. Therefore, knowledge of the structure of non-Ideal pulsar magnetospheres is important because their comparison (including models fo"},"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":"1108.2138","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-08-10T10:16:43Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"1bc378461c8d45c6e8c67378a945cf82e59dfc6e5ce1a5dec69b1d557544c67a","abstract_canon_sha256":"b996fa52202847b875f92ac384ec58de558b0ec9b99bf45f06183011863b4305"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:55.737552Z","signature_b64":"81dAk2L8WVNV3SbuLLDyDzwuu4nbxknPfqS8WMrOPCFfNHlY9tNSJQKN2LMUBqmKMxzvJSD1s4aHhXem/QWVDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d43da4da34d4ee6b913f93af622dcdb6b2a7cdecfe53474a4145daeec222785","last_reissued_at":"2026-05-18T02:00:55.736884Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:55.736884Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Toward a Realistic Pulsar Magnetosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"Alice Harding, Constantinos Kalapotharakos, Demosthenes Kazanas, Ioannis Contopoulos","submitted_at":"2011-08-10T10:16:43Z","abstract_excerpt":"We present the magnetic and electric field structures as well as the currents and charge densities of pulsar magnetospheres which do not obey the ideal condition, ${\\bf E \\cdot B =0}$. Since the acceleration of particles and the production of radiation requires the presence of an electric field component parallel to the magnetic field, ${\\bf E}_\\parallel$, the structure of non-Ideal pulsar magnetospheres is intimately related to the production of pulsar radiation. Therefore, knowledge of the structure of non-Ideal pulsar magnetospheres is important because their comparison (including models fo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.2138","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":"1108.2138","created_at":"2026-05-18T02:00:55.736983+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.2138v2","created_at":"2026-05-18T02:00:55.736983+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.2138","created_at":"2026-05-18T02:00:55.736983+00:00"},{"alias_kind":"pith_short_12","alias_value":"TVB5UTNDJVHO","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_16","alias_value":"TVB5UTNDJVHONOIT","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_8","alias_value":"TVB5UTND","created_at":"2026-05-18T12:26:42.757692+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/TVB5UTNDJVHONOIT7E5PMIW43N","json":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N.json","graph_json":"https://pith.science/api/pith-number/TVB5UTNDJVHONOIT7E5PMIW43N/graph.json","events_json":"https://pith.science/api/pith-number/TVB5UTNDJVHONOIT7E5PMIW43N/events.json","paper":"https://pith.science/paper/TVB5UTND"},"agent_actions":{"view_html":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N","download_json":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N.json","view_paper":"https://pith.science/paper/TVB5UTND","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.2138&json=true","fetch_graph":"https://pith.science/api/pith-number/TVB5UTNDJVHONOIT7E5PMIW43N/graph.json","fetch_events":"https://pith.science/api/pith-number/TVB5UTNDJVHONOIT7E5PMIW43N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N/action/storage_attestation","attest_author":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N/action/author_attestation","sign_citation":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N/action/citation_signature","submit_replication":"https://pith.science/pith/TVB5UTNDJVHONOIT7E5PMIW43N/action/replication_record"}},"created_at":"2026-05-18T02:00:55.736983+00:00","updated_at":"2026-05-18T02:00:55.736983+00:00"}