{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FPSJ27IRBGP5HCSK5GTHJ63SGY","short_pith_number":"pith:FPSJ27IR","schema_version":"1.0","canonical_sha256":"2be49d7d11099fd38a4ae9a674fb723601b428b15cf7ec59818d24b2ca3b989a","source":{"kind":"arxiv","id":"1406.0301","version":2},"attestation_state":"computed","paper":{"title":"The role of pressure gradients in driving sunward magnetosheath flows and magnetopause motion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.geo-ph","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"D. L. Turner, J. P. Eastwood, M. O. Archer, S. J. Schwartz, T. S. Horbury","submitted_at":"2014-06-02T09:10:09Z","abstract_excerpt":"While pressure balance can predict how far the magnetopause will move in response to an upstream pressure change, it cannot determine how fast the transient reponse will be. Using Time History of Events and Macroscale Interactions during Substorms (THEMIS), we present multipoint observations revealing, for the first time, strong (thermal + magnetic) pressure gradients in the magnetosheath due to a foreshock transient, most likely a Hot Flow Anomaly (HFA), which decreased the total pressure upstream of the bow shock. By converting the spacecraft time series into a spatial picture, we quantitati"},"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":"1406.0301","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2014-06-02T09:10:09Z","cross_cats_sorted":["physics.geo-ph","physics.plasm-ph"],"title_canon_sha256":"e55e2c09a1cc87d2ac0b8749b0d948d9d8dfce6fbe12601c629c10c8cd87bf86","abstract_canon_sha256":"ffeb7804ce570756c062c9389d00859fed103c13875f7b497dfe4b9b2bec6c65"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:34:52.230374Z","signature_b64":"WKcSf8TKTK20NP2xPt90W+/Akv/7JZLa6VTcA8VKNdHfgTWYLjlo8NjK+Hewaz4AcyIpBLC3lSO9B0Pd8oNLCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2be49d7d11099fd38a4ae9a674fb723601b428b15cf7ec59818d24b2ca3b989a","last_reissued_at":"2026-05-18T02:34:52.230011Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:34:52.230011Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The role of pressure gradients in driving sunward magnetosheath flows and magnetopause motion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.geo-ph","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"D. L. Turner, J. P. Eastwood, M. O. Archer, S. J. Schwartz, T. S. Horbury","submitted_at":"2014-06-02T09:10:09Z","abstract_excerpt":"While pressure balance can predict how far the magnetopause will move in response to an upstream pressure change, it cannot determine how fast the transient reponse will be. Using Time History of Events and Macroscale Interactions during Substorms (THEMIS), we present multipoint observations revealing, for the first time, strong (thermal + magnetic) pressure gradients in the magnetosheath due to a foreshock transient, most likely a Hot Flow Anomaly (HFA), which decreased the total pressure upstream of the bow shock. By converting the spacecraft time series into a spatial picture, we quantitati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.0301","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":"1406.0301","created_at":"2026-05-18T02:34:52.230067+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.0301v2","created_at":"2026-05-18T02:34:52.230067+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.0301","created_at":"2026-05-18T02:34:52.230067+00:00"},{"alias_kind":"pith_short_12","alias_value":"FPSJ27IRBGP5","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FPSJ27IRBGP5HCSK","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FPSJ27IR","created_at":"2026-05-18T12:28:28.263976+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/FPSJ27IRBGP5HCSK5GTHJ63SGY","json":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY.json","graph_json":"https://pith.science/api/pith-number/FPSJ27IRBGP5HCSK5GTHJ63SGY/graph.json","events_json":"https://pith.science/api/pith-number/FPSJ27IRBGP5HCSK5GTHJ63SGY/events.json","paper":"https://pith.science/paper/FPSJ27IR"},"agent_actions":{"view_html":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY","download_json":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY.json","view_paper":"https://pith.science/paper/FPSJ27IR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.0301&json=true","fetch_graph":"https://pith.science/api/pith-number/FPSJ27IRBGP5HCSK5GTHJ63SGY/graph.json","fetch_events":"https://pith.science/api/pith-number/FPSJ27IRBGP5HCSK5GTHJ63SGY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY/action/storage_attestation","attest_author":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY/action/author_attestation","sign_citation":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY/action/citation_signature","submit_replication":"https://pith.science/pith/FPSJ27IRBGP5HCSK5GTHJ63SGY/action/replication_record"}},"created_at":"2026-05-18T02:34:52.230067+00:00","updated_at":"2026-05-18T02:34:52.230067+00:00"}