{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:KIPSQJELL2KS3QGIDWHBFZWU5I","short_pith_number":"pith:KIPSQJEL","schema_version":"1.0","canonical_sha256":"521f28248b5e952dc0c81d8e12e6d4ea33738f7395724145fa46be4f6399ec3b","source":{"kind":"arxiv","id":"1603.04900","version":1},"attestation_state":"computed","paper":{"title":"A Numerical Study of Long-Range Magnetic Impacts during Coronal Mass Ejections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. M. Title, C. J. Schrijver, M. C. M. Cheung, M. Jin, M. L. Derosa, N. V. Nitta","submitted_at":"2016-03-15T22:08:43Z","abstract_excerpt":"With the global view and high-cadence observations from SDO/AIA and STEREO, many spatially separated solar eruptive events appear to be coupled. However, the mechanisms for \"sympathetic\" events are still largely unknown. In this study, we investigate the impact of an erupting flux rope on surrounding solar structures through large-scale magnetic coupling. We build a realistic environment of the solar corona on 2011 February 15 using a global magnetohydrodynamics (MHD) model and initiate coronal mass ejections (CMEs) in active region (AR) 11158 by inserting Gibson-Low analytical flux ropes. We "},"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":"1603.04900","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-03-15T22:08:43Z","cross_cats_sorted":[],"title_canon_sha256":"816f6677b0d54b1619b7dbb1be57b65a897b99d713a533392844908270cbe5d2","abstract_canon_sha256":"1394e19a0ebe7ecaedff8208da6d4cdc8a7b346b1086fd8b6741dcb6e5977ff5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:59.730889Z","signature_b64":"aFMSitd1zShiCfsfTcoAqP3sMrx07XfLk+diDpmyZJyCKmRHQnBTWadfTnt9qcLPqGx64P2KLF0KDF2aLDPKCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"521f28248b5e952dc0c81d8e12e6d4ea33738f7395724145fa46be4f6399ec3b","last_reissued_at":"2026-05-18T01:18:59.730176Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:59.730176Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Numerical Study of Long-Range Magnetic Impacts during Coronal Mass Ejections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. M. Title, C. J. Schrijver, M. C. M. Cheung, M. Jin, M. L. Derosa, N. V. Nitta","submitted_at":"2016-03-15T22:08:43Z","abstract_excerpt":"With the global view and high-cadence observations from SDO/AIA and STEREO, many spatially separated solar eruptive events appear to be coupled. However, the mechanisms for \"sympathetic\" events are still largely unknown. In this study, we investigate the impact of an erupting flux rope on surrounding solar structures through large-scale magnetic coupling. We build a realistic environment of the solar corona on 2011 February 15 using a global magnetohydrodynamics (MHD) model and initiate coronal mass ejections (CMEs) in active region (AR) 11158 by inserting Gibson-Low analytical flux ropes. We "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.04900","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":"1603.04900","created_at":"2026-05-18T01:18:59.730323+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.04900v1","created_at":"2026-05-18T01:18:59.730323+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.04900","created_at":"2026-05-18T01:18:59.730323+00:00"},{"alias_kind":"pith_short_12","alias_value":"KIPSQJELL2KS","created_at":"2026-05-18T12:30:25.849896+00:00"},{"alias_kind":"pith_short_16","alias_value":"KIPSQJELL2KS3QGI","created_at":"2026-05-18T12:30:25.849896+00:00"},{"alias_kind":"pith_short_8","alias_value":"KIPSQJEL","created_at":"2026-05-18T12:30:25.849896+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/KIPSQJELL2KS3QGIDWHBFZWU5I","json":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I.json","graph_json":"https://pith.science/api/pith-number/KIPSQJELL2KS3QGIDWHBFZWU5I/graph.json","events_json":"https://pith.science/api/pith-number/KIPSQJELL2KS3QGIDWHBFZWU5I/events.json","paper":"https://pith.science/paper/KIPSQJEL"},"agent_actions":{"view_html":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I","download_json":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I.json","view_paper":"https://pith.science/paper/KIPSQJEL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.04900&json=true","fetch_graph":"https://pith.science/api/pith-number/KIPSQJELL2KS3QGIDWHBFZWU5I/graph.json","fetch_events":"https://pith.science/api/pith-number/KIPSQJELL2KS3QGIDWHBFZWU5I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I/action/storage_attestation","attest_author":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I/action/author_attestation","sign_citation":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I/action/citation_signature","submit_replication":"https://pith.science/pith/KIPSQJELL2KS3QGIDWHBFZWU5I/action/replication_record"}},"created_at":"2026-05-18T01:18:59.730323+00:00","updated_at":"2026-05-18T01:18:59.730323+00:00"}