{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:NPHB3QZW653V3EADDBDKLPRUVF","short_pith_number":"pith:NPHB3QZW","schema_version":"1.0","canonical_sha256":"6bce1dc336f7775d90031846a5be34a94f75085fd7e3255ae1fd1c87b8df4c1a","source":{"kind":"arxiv","id":"1607.05533","version":1},"attestation_state":"computed","paper":{"title":"Comparison of CME/shock propagation models with heliospheric imaging and in situ observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Bernd Inhester, Lei Lu, Thomas Wiegelmann, Xinhua Zhao, Xueshang Feng, Ying D. Liu","submitted_at":"2016-07-19T11:44:02Z","abstract_excerpt":"The prediction of the arrival time for fast coronal mass ejections (CMEs) and their associated shocks is highly desirable in space weather studies. In this paper, we use two shock propagation models, i.e. Data Guided Shock Time Of Arrival (DGSTOA) and Data Guided Shock Propagation Model (DGSPM), to predict the kinematical evolution of interplanetary shocks associated with fast CMEs. DGSTOA is based on the similarity theory of shock waves in the solar wind reference frame, and DGSPM on the non-similarity theory in the stationary reference frame. The inputs are the kinematics of the CME front at"},"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":"1607.05533","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-07-19T11:44:02Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"a71b2377bae0eb66e791bdc82cf5c181bd961193019e35f7ee0d2d17926a6898","abstract_canon_sha256":"0223f43edadfb1e1f6b1546178f9520c0a839ac3dce9db8ec1e572be09a4ee26"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:02:00.230504Z","signature_b64":"/1W9pGCRGEzvoLDDGzeSZRyctj1gspgf4d3cLzunooxd8DX4mFO2XpVaplXWPOANGGwdims2cKZJF+gXtG1uBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6bce1dc336f7775d90031846a5be34a94f75085fd7e3255ae1fd1c87b8df4c1a","last_reissued_at":"2026-05-18T01:02:00.229860Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:02:00.229860Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comparison of CME/shock propagation models with heliospheric imaging and in situ observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Bernd Inhester, Lei Lu, Thomas Wiegelmann, Xinhua Zhao, Xueshang Feng, Ying D. Liu","submitted_at":"2016-07-19T11:44:02Z","abstract_excerpt":"The prediction of the arrival time for fast coronal mass ejections (CMEs) and their associated shocks is highly desirable in space weather studies. In this paper, we use two shock propagation models, i.e. Data Guided Shock Time Of Arrival (DGSTOA) and Data Guided Shock Propagation Model (DGSPM), to predict the kinematical evolution of interplanetary shocks associated with fast CMEs. DGSTOA is based on the similarity theory of shock waves in the solar wind reference frame, and DGSPM on the non-similarity theory in the stationary reference frame. The inputs are the kinematics of the CME front at"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.05533","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":"1607.05533","created_at":"2026-05-18T01:02:00.229968+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.05533v1","created_at":"2026-05-18T01:02:00.229968+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.05533","created_at":"2026-05-18T01:02:00.229968+00:00"},{"alias_kind":"pith_short_12","alias_value":"NPHB3QZW653V","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"NPHB3QZW653V3EAD","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"NPHB3QZW","created_at":"2026-05-18T12:30:36.002864+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/NPHB3QZW653V3EADDBDKLPRUVF","json":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF.json","graph_json":"https://pith.science/api/pith-number/NPHB3QZW653V3EADDBDKLPRUVF/graph.json","events_json":"https://pith.science/api/pith-number/NPHB3QZW653V3EADDBDKLPRUVF/events.json","paper":"https://pith.science/paper/NPHB3QZW"},"agent_actions":{"view_html":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF","download_json":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF.json","view_paper":"https://pith.science/paper/NPHB3QZW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.05533&json=true","fetch_graph":"https://pith.science/api/pith-number/NPHB3QZW653V3EADDBDKLPRUVF/graph.json","fetch_events":"https://pith.science/api/pith-number/NPHB3QZW653V3EADDBDKLPRUVF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF/action/storage_attestation","attest_author":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF/action/author_attestation","sign_citation":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF/action/citation_signature","submit_replication":"https://pith.science/pith/NPHB3QZW653V3EADDBDKLPRUVF/action/replication_record"}},"created_at":"2026-05-18T01:02:00.229968+00:00","updated_at":"2026-05-18T01:02:00.229968+00:00"}