{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:UHCKWDRHM2ILRXCDXL2SOJ4YES","short_pith_number":"pith:UHCKWDRH","schema_version":"1.0","canonical_sha256":"a1c4ab0e276690b8dc43baf5272798248ae5c7a458566d4d11930066efe01951","source":{"kind":"arxiv","id":"1708.08818","version":1},"attestation_state":"computed","paper":{"title":"Large-scale solar wind flow around Saturn's nonaxisymmetric magnetosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.space-ph","authors_text":"A. H. Sulaiman, D. A. Gurnett, N. Achilleos, N. Sergis, W. S. Kurth, X. Jia","submitted_at":"2017-08-29T15:20:53Z","abstract_excerpt":"The interaction between the solar wind and a magnetosphere is fundamental to the dynamics of a planetary system. Here, we address fundamental questions on the large-scale magnetosheath flow around Saturn using a 3D magnetohydrodynamic (MHD) simulation. We find Saturn's polar-flattened magnetosphere to channel ~20% more flow over the poles than around the flanks at the terminator. Further, we decompose the MHD forces responsible for accelerating the magnetosheath plasma to find the plasma pressure gradient as the dominant driver. This is by virtue of a high-beta magnetosheath, and in turn, 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":"1708.08818","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2017-08-29T15:20:53Z","cross_cats_sorted":[],"title_canon_sha256":"67bc5f1b7ba34b83440990e084a17f642fa1498ad51d65baab582af9f3a6cbd3","abstract_canon_sha256":"6842f7b958682501f1ed50c9a5c8fe405ce17e8950708fcf57462336bcd7d4b0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:25.546044Z","signature_b64":"PpjwfZ8rxcLeU8RftvLbvlahqnwClPOXZyxlemXFON18SzUruKLrj0cBFNaX0QJsGtKT91OF6DqTojeI1c7yDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a1c4ab0e276690b8dc43baf5272798248ae5c7a458566d4d11930066efe01951","last_reissued_at":"2026-05-18T00:36:25.545221Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:25.545221Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Large-scale solar wind flow around Saturn's nonaxisymmetric magnetosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.space-ph","authors_text":"A. H. Sulaiman, D. A. Gurnett, N. Achilleos, N. Sergis, W. S. Kurth, X. Jia","submitted_at":"2017-08-29T15:20:53Z","abstract_excerpt":"The interaction between the solar wind and a magnetosphere is fundamental to the dynamics of a planetary system. Here, we address fundamental questions on the large-scale magnetosheath flow around Saturn using a 3D magnetohydrodynamic (MHD) simulation. We find Saturn's polar-flattened magnetosphere to channel ~20% more flow over the poles than around the flanks at the terminator. Further, we decompose the MHD forces responsible for accelerating the magnetosheath plasma to find the plasma pressure gradient as the dominant driver. This is by virtue of a high-beta magnetosheath, and in turn, the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.08818","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":"1708.08818","created_at":"2026-05-18T00:36:25.545358+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.08818v1","created_at":"2026-05-18T00:36:25.545358+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.08818","created_at":"2026-05-18T00:36:25.545358+00:00"},{"alias_kind":"pith_short_12","alias_value":"UHCKWDRHM2IL","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_16","alias_value":"UHCKWDRHM2ILRXCD","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_8","alias_value":"UHCKWDRH","created_at":"2026-05-18T12:31:46.661854+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/UHCKWDRHM2ILRXCDXL2SOJ4YES","json":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES.json","graph_json":"https://pith.science/api/pith-number/UHCKWDRHM2ILRXCDXL2SOJ4YES/graph.json","events_json":"https://pith.science/api/pith-number/UHCKWDRHM2ILRXCDXL2SOJ4YES/events.json","paper":"https://pith.science/paper/UHCKWDRH"},"agent_actions":{"view_html":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES","download_json":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES.json","view_paper":"https://pith.science/paper/UHCKWDRH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.08818&json=true","fetch_graph":"https://pith.science/api/pith-number/UHCKWDRHM2ILRXCDXL2SOJ4YES/graph.json","fetch_events":"https://pith.science/api/pith-number/UHCKWDRHM2ILRXCDXL2SOJ4YES/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES/action/storage_attestation","attest_author":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES/action/author_attestation","sign_citation":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES/action/citation_signature","submit_replication":"https://pith.science/pith/UHCKWDRHM2ILRXCDXL2SOJ4YES/action/replication_record"}},"created_at":"2026-05-18T00:36:25.545358+00:00","updated_at":"2026-05-18T00:36:25.545358+00:00"}