{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:DTOU5MQVRYP7DYRVVEMU2TW3NG","short_pith_number":"pith:DTOU5MQV","schema_version":"1.0","canonical_sha256":"1cdd4eb2158e1ff1e235a9194d4edb69a7dd794f67e7f10dfd72a0d0dff19fe5","source":{"kind":"arxiv","id":"1703.10562","version":1},"attestation_state":"computed","paper":{"title":"Relative magnetic helicity as a diagnostic of solar eruptivity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"E. Pariat, F. P. Zuccarello, G. Valori, J. E. Leake, K. Dalmasse, M. G. Linton","submitted_at":"2017-03-30T16:51:09Z","abstract_excerpt":"The discovery of clear criteria that can deterministically describe the eruptive state of a solar active region would lead to major improvements on space weather predictions. Using series of numerical simulations of the emergence of a magnetic flux rope in a magnetized coronal, leading either to eruptions or to stable configurations, we test several global scalar quantities for the ability to discriminate between the eruptive and the non-eruptive simulations. From the magnetic field generated by the three-dimensional magnetohydrodynamical simulations, we compute and analyse the evolution of th"},"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":"1703.10562","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-03-30T16:51:09Z","cross_cats_sorted":[],"title_canon_sha256":"ddac39dec89177ef2afbacbab875670ea86e4cfa4a8f518bab86f36402fa3833","abstract_canon_sha256":"288cf7acfbeab587c3b0d6fe45e0ffc60e2991213fd301aa53ba018fa77b4b80"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:44:23.205748Z","signature_b64":"XdN0nUp9AbtR/9/TgOIpN9pgHm4OKVn6MrLJgiWNaznbEsAt1WZPTOBZVX0sl0fxsZd/6Q6fD6L+f3xL/+DRDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1cdd4eb2158e1ff1e235a9194d4edb69a7dd794f67e7f10dfd72a0d0dff19fe5","last_reissued_at":"2026-05-18T00:44:23.205222Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:44:23.205222Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relative magnetic helicity as a diagnostic of solar eruptivity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"E. Pariat, F. P. Zuccarello, G. Valori, J. E. Leake, K. Dalmasse, M. G. Linton","submitted_at":"2017-03-30T16:51:09Z","abstract_excerpt":"The discovery of clear criteria that can deterministically describe the eruptive state of a solar active region would lead to major improvements on space weather predictions. Using series of numerical simulations of the emergence of a magnetic flux rope in a magnetized coronal, leading either to eruptions or to stable configurations, we test several global scalar quantities for the ability to discriminate between the eruptive and the non-eruptive simulations. From the magnetic field generated by the three-dimensional magnetohydrodynamical simulations, we compute and analyse the evolution of th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.10562","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":"1703.10562","created_at":"2026-05-18T00:44:23.205302+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.10562v1","created_at":"2026-05-18T00:44:23.205302+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.10562","created_at":"2026-05-18T00:44:23.205302+00:00"},{"alias_kind":"pith_short_12","alias_value":"DTOU5MQVRYP7","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_16","alias_value":"DTOU5MQVRYP7DYRV","created_at":"2026-05-18T12:31:12.930513+00:00"},{"alias_kind":"pith_short_8","alias_value":"DTOU5MQV","created_at":"2026-05-18T12:31:12.930513+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/DTOU5MQVRYP7DYRVVEMU2TW3NG","json":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG.json","graph_json":"https://pith.science/api/pith-number/DTOU5MQVRYP7DYRVVEMU2TW3NG/graph.json","events_json":"https://pith.science/api/pith-number/DTOU5MQVRYP7DYRVVEMU2TW3NG/events.json","paper":"https://pith.science/paper/DTOU5MQV"},"agent_actions":{"view_html":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG","download_json":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG.json","view_paper":"https://pith.science/paper/DTOU5MQV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.10562&json=true","fetch_graph":"https://pith.science/api/pith-number/DTOU5MQVRYP7DYRVVEMU2TW3NG/graph.json","fetch_events":"https://pith.science/api/pith-number/DTOU5MQVRYP7DYRVVEMU2TW3NG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG/action/storage_attestation","attest_author":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG/action/author_attestation","sign_citation":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG/action/citation_signature","submit_replication":"https://pith.science/pith/DTOU5MQVRYP7DYRVVEMU2TW3NG/action/replication_record"}},"created_at":"2026-05-18T00:44:23.205302+00:00","updated_at":"2026-05-18T00:44:23.205302+00:00"}