{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:MDMERUBI2Q3EE3ASQU5AVKZJ7J","short_pith_number":"pith:MDMERUBI","schema_version":"1.0","canonical_sha256":"60d848d028d436426c12853a0aab29fa44e96cbc0ac8645f9748c829fe8abf71","source":{"kind":"arxiv","id":"1705.08198","version":2},"attestation_state":"computed","paper":{"title":"Origin and Structures of Solar Eruptions I: Magnetic Flux Rope (Invited Review)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"M. D. Ding, X. Cheng, Y. Guo","submitted_at":"2017-05-23T12:01:40Z","abstract_excerpt":"Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic eruptive phenomena in our solar system and able to release a large quantity of plasma and magnetic flux from the solar atmosphere into the solar wind. When these high-speed magnetized plasmas along with the energetic particles arrive at the Earth, they may interact with the magnetosphere and ionosphere, and seriously affect the safety of human high-tech activities in outer space. The travel time of a CME to 1 AU is about 1-3 days, while energetic particles from the eruptions arrive even earlier. An efficient "},"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":"1705.08198","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-05-23T12:01:40Z","cross_cats_sorted":["physics.plasm-ph","physics.space-ph"],"title_canon_sha256":"e75f08f4d20d3d2c87c0592d0c20ea529bf7c7155c4530a20e289dcf1eba3d7b","abstract_canon_sha256":"e1bf1ca144d8ff9b3de4b3d6ff2705f876530c2afe2b69c67008e3cc548bb08e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:28.349515Z","signature_b64":"+saU5BpKxvoFj81wFdyvpc3vhB2pFfrT6xZI6Eyfbms0tR5l2gm61iKoEcGNFEsAvdOlOgsCDTEuatwMK1wJBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"60d848d028d436426c12853a0aab29fa44e96cbc0ac8645f9748c829fe8abf71","last_reissued_at":"2026-05-18T00:40:28.348947Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:28.348947Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Origin and Structures of Solar Eruptions I: Magnetic Flux Rope (Invited Review)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"M. D. Ding, X. Cheng, Y. Guo","submitted_at":"2017-05-23T12:01:40Z","abstract_excerpt":"Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic eruptive phenomena in our solar system and able to release a large quantity of plasma and magnetic flux from the solar atmosphere into the solar wind. When these high-speed magnetized plasmas along with the energetic particles arrive at the Earth, they may interact with the magnetosphere and ionosphere, and seriously affect the safety of human high-tech activities in outer space. The travel time of a CME to 1 AU is about 1-3 days, while energetic particles from the eruptions arrive even earlier. An efficient "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.08198","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":"1705.08198","created_at":"2026-05-18T00:40:28.349026+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.08198v2","created_at":"2026-05-18T00:40:28.349026+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.08198","created_at":"2026-05-18T00:40:28.349026+00:00"},{"alias_kind":"pith_short_12","alias_value":"MDMERUBI2Q3E","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_16","alias_value":"MDMERUBI2Q3EE3AS","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_8","alias_value":"MDMERUBI","created_at":"2026-05-18T12:31:31.346846+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/MDMERUBI2Q3EE3ASQU5AVKZJ7J","json":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J.json","graph_json":"https://pith.science/api/pith-number/MDMERUBI2Q3EE3ASQU5AVKZJ7J/graph.json","events_json":"https://pith.science/api/pith-number/MDMERUBI2Q3EE3ASQU5AVKZJ7J/events.json","paper":"https://pith.science/paper/MDMERUBI"},"agent_actions":{"view_html":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J","download_json":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J.json","view_paper":"https://pith.science/paper/MDMERUBI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.08198&json=true","fetch_graph":"https://pith.science/api/pith-number/MDMERUBI2Q3EE3ASQU5AVKZJ7J/graph.json","fetch_events":"https://pith.science/api/pith-number/MDMERUBI2Q3EE3ASQU5AVKZJ7J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J/action/storage_attestation","attest_author":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J/action/author_attestation","sign_citation":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J/action/citation_signature","submit_replication":"https://pith.science/pith/MDMERUBI2Q3EE3ASQU5AVKZJ7J/action/replication_record"}},"created_at":"2026-05-18T00:40:28.349026+00:00","updated_at":"2026-05-18T00:40:28.349026+00:00"}