{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SJC32DJKWW54XYBLODHNG2HOOX","short_pith_number":"pith:SJC32DJK","schema_version":"1.0","canonical_sha256":"9245bd0d2ab5bbcbe02b70ced368ee75c952032d2afbf9640674f16e33a7371e","source":{"kind":"arxiv","id":"1312.1865","version":1},"attestation_state":"computed","paper":{"title":"Study of the solar wind-magnetosphere coupling on different time scales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","physics.data-an","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Badruddin, O.P.M. Aslam","submitted_at":"2013-12-05T18:50:40Z","abstract_excerpt":"Solar wind-magnetosphere coupling, its causes and consequences have been studied for the last several decades. However, the assessment of continuously changing behaviour of the sun, plasma and field flows in the interplanetary space and their influence on geomagnetic activity is still a subject of intense research. Search for the best possible coupling function is also important for space weather prediction. We utilize four geomagnetic indices (ap, aa, AE and Dst) as parameters of geomagnetic activity level in the earth's magnetosphere. In addition to these indices, we utilize various solar wi"},"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":"1312.1865","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-12-05T18:50:40Z","cross_cats_sorted":["astro-ph.EP","physics.data-an","physics.space-ph"],"title_canon_sha256":"effd2a6a0c894cee2b3c14ba842d393401d418bdfe30c2df234a3109ccca7976","abstract_canon_sha256":"b6fcd4f97b341cd7a41fee982a7e31b09c36875a44cfd1b4c73d78a4f0c55f96"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:05:19.579778Z","signature_b64":"Ge8Z14SW+pG0fXQIwN3C+0ktQID4gpmtpY4Xo5vzgezTG9iDhAzcE8f0iy97QYh9U6kYS+hNIHBT/jtQc2CZCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9245bd0d2ab5bbcbe02b70ced368ee75c952032d2afbf9640674f16e33a7371e","last_reissued_at":"2026-05-18T03:05:19.579296Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:05:19.579296Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Study of the solar wind-magnetosphere coupling on different time scales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","physics.data-an","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Badruddin, O.P.M. Aslam","submitted_at":"2013-12-05T18:50:40Z","abstract_excerpt":"Solar wind-magnetosphere coupling, its causes and consequences have been studied for the last several decades. However, the assessment of continuously changing behaviour of the sun, plasma and field flows in the interplanetary space and their influence on geomagnetic activity is still a subject of intense research. Search for the best possible coupling function is also important for space weather prediction. We utilize four geomagnetic indices (ap, aa, AE and Dst) as parameters of geomagnetic activity level in the earth's magnetosphere. In addition to these indices, we utilize various solar wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.1865","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":"1312.1865","created_at":"2026-05-18T03:05:19.579385+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.1865v1","created_at":"2026-05-18T03:05:19.579385+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.1865","created_at":"2026-05-18T03:05:19.579385+00:00"},{"alias_kind":"pith_short_12","alias_value":"SJC32DJKWW54","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SJC32DJKWW54XYBL","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SJC32DJK","created_at":"2026-05-18T12:27:59.945178+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/SJC32DJKWW54XYBLODHNG2HOOX","json":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX.json","graph_json":"https://pith.science/api/pith-number/SJC32DJKWW54XYBLODHNG2HOOX/graph.json","events_json":"https://pith.science/api/pith-number/SJC32DJKWW54XYBLODHNG2HOOX/events.json","paper":"https://pith.science/paper/SJC32DJK"},"agent_actions":{"view_html":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX","download_json":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX.json","view_paper":"https://pith.science/paper/SJC32DJK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.1865&json=true","fetch_graph":"https://pith.science/api/pith-number/SJC32DJKWW54XYBLODHNG2HOOX/graph.json","fetch_events":"https://pith.science/api/pith-number/SJC32DJKWW54XYBLODHNG2HOOX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX/action/storage_attestation","attest_author":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX/action/author_attestation","sign_citation":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX/action/citation_signature","submit_replication":"https://pith.science/pith/SJC32DJKWW54XYBLODHNG2HOOX/action/replication_record"}},"created_at":"2026-05-18T03:05:19.579385+00:00","updated_at":"2026-05-18T03:05:19.579385+00:00"}