{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:LBWH6FHGLGT3GOI5BGOR37JIDV","short_pith_number":"pith:LBWH6FHG","schema_version":"1.0","canonical_sha256":"586c7f14e659a7b3391d099d1dfd281d6b9e65d3f4796c4634af15cb0db5bb99","source":{"kind":"arxiv","id":"1606.01074","version":1},"attestation_state":"computed","paper":{"title":"How the IMF $\\mathit{B}_{y}$ induces a $\\mathit{B}_{y}$ component in the closed magnetosphere and how it leads to asymmetric currents and convection patterns in the two hemispheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.space-ph","authors_text":"J. P. Reistad, K.M. Laundal, K. Snekvik, N. {\\O}stgaard, P. Tenfjord, S. E. Milan, S. Haaland","submitted_at":"2016-06-03T13:05:38Z","abstract_excerpt":"We used the Lyon-Fedder-Mobarry global magnetohydrodynamics model to study the effects of the interplanetary magnetic field (IMF) IMF $\\mathit{B}_{y}$ component on the coupling between the solar wind and magnetosphere-ionosphere system. When the IMF reconnects with the terrestrial magnetic field with IMF $\\mathit{B}_{y}$ $\\neq$ 0, flux transport is asymmetrically distributed between the two hemispheres. We describe how $\\mathit{B}_{y}$ is induced in the closed magnetosphere on both the dayside and nightside and present the governing equations. The magnetosphere imposes asymmetric forces on the"},"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":"1606.01074","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2016-06-03T13:05:38Z","cross_cats_sorted":[],"title_canon_sha256":"05cad7e60b2bd295a8dacbfa16fdf4d0cc5bf7f320614b3f9b71d6d6308c40ca","abstract_canon_sha256":"aed083c1d67fad3b704acd45194df9a316cb52fb38fa7e386553fcd563d5ad17"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:59.311683Z","signature_b64":"i26GNKgM+CWHnxv+Pp4CUfdh70qrSy8SYo1Vm86ShTOdmAexetUByLaL0UHzhLSF1USKymHuB6xkAkE/qVscDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"586c7f14e659a7b3391d099d1dfd281d6b9e65d3f4796c4634af15cb0db5bb99","last_reissued_at":"2026-05-18T01:12:59.311338Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:59.311338Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"How the IMF $\\mathit{B}_{y}$ induces a $\\mathit{B}_{y}$ component in the closed magnetosphere and how it leads to asymmetric currents and convection patterns in the two hemispheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.space-ph","authors_text":"J. P. Reistad, K.M. Laundal, K. Snekvik, N. {\\O}stgaard, P. Tenfjord, S. E. Milan, S. Haaland","submitted_at":"2016-06-03T13:05:38Z","abstract_excerpt":"We used the Lyon-Fedder-Mobarry global magnetohydrodynamics model to study the effects of the interplanetary magnetic field (IMF) IMF $\\mathit{B}_{y}$ component on the coupling between the solar wind and magnetosphere-ionosphere system. When the IMF reconnects with the terrestrial magnetic field with IMF $\\mathit{B}_{y}$ $\\neq$ 0, flux transport is asymmetrically distributed between the two hemispheres. We describe how $\\mathit{B}_{y}$ is induced in the closed magnetosphere on both the dayside and nightside and present the governing equations. The magnetosphere imposes asymmetric forces on the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.01074","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":"1606.01074","created_at":"2026-05-18T01:12:59.311394+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.01074v1","created_at":"2026-05-18T01:12:59.311394+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.01074","created_at":"2026-05-18T01:12:59.311394+00:00"},{"alias_kind":"pith_short_12","alias_value":"LBWH6FHGLGT3","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_16","alias_value":"LBWH6FHGLGT3GOI5","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_8","alias_value":"LBWH6FHG","created_at":"2026-05-18T12:30:29.479603+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/LBWH6FHGLGT3GOI5BGOR37JIDV","json":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV.json","graph_json":"https://pith.science/api/pith-number/LBWH6FHGLGT3GOI5BGOR37JIDV/graph.json","events_json":"https://pith.science/api/pith-number/LBWH6FHGLGT3GOI5BGOR37JIDV/events.json","paper":"https://pith.science/paper/LBWH6FHG"},"agent_actions":{"view_html":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV","download_json":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV.json","view_paper":"https://pith.science/paper/LBWH6FHG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.01074&json=true","fetch_graph":"https://pith.science/api/pith-number/LBWH6FHGLGT3GOI5BGOR37JIDV/graph.json","fetch_events":"https://pith.science/api/pith-number/LBWH6FHGLGT3GOI5BGOR37JIDV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV/action/storage_attestation","attest_author":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV/action/author_attestation","sign_citation":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV/action/citation_signature","submit_replication":"https://pith.science/pith/LBWH6FHGLGT3GOI5BGOR37JIDV/action/replication_record"}},"created_at":"2026-05-18T01:12:59.311394+00:00","updated_at":"2026-05-18T01:12:59.311394+00:00"}