{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:R2NUEJO52C2JTD4BLMCVISDGCN","short_pith_number":"pith:R2NUEJO5","schema_version":"1.0","canonical_sha256":"8e9b4225ddd0b4998f815b05544866135240a8f555e45f557d94d403408e16e3","source":{"kind":"arxiv","id":"1701.06440","version":1},"attestation_state":"computed","paper":{"title":"Plasma flows and magnetic field interplay during the formation of a pore","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Cristaldi, A. Tritschler, F. Giannattasio, F. Giorgi, F. Zuccarello, I. Ermolli, M. Stangalini, P. Romano","submitted_at":"2017-01-23T15:11:19Z","abstract_excerpt":"We studied the formation of a pore in AR NOAA 11462. We analysed data obtained with the IBIS at the DST on April 17, 2012, consisting of full Stokes measurements of the Fe I 617.3 nm lines. Furthermore, we analysed SDO/HMI observations in the continuum and vector magnetograms derived from the Fe I 617.3 nm line data taken from April 15 to 19, 2012. We estimated the magnetic field strength and vector components and the LOS and horizontal motions in the photospheric region hosting the pore formation. We discuss our results in light of other observational studies and recent advances of numerical "},"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":"1701.06440","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-01-23T15:11:19Z","cross_cats_sorted":[],"title_canon_sha256":"188adc097f3f8631bfba774d3c11b7d97da5a17bb0c70ddfacb8f5fd119e6f25","abstract_canon_sha256":"2f28ce80531979e0ba1d1796a110ab3c78b5625fc0a7e96bdec156861bf2677e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:18.375564Z","signature_b64":"rgAjW0p5tAdnhfNueJc3do7kx91IMc5bwB9GiuM5CEjJDeSd7xerWaGfIY2Q5SV9w1vnUo07Sah4WL39XOXiCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8e9b4225ddd0b4998f815b05544866135240a8f555e45f557d94d403408e16e3","last_reissued_at":"2026-05-18T00:52:18.374977Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:18.374977Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Plasma flows and magnetic field interplay during the formation of a pore","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Cristaldi, A. Tritschler, F. Giannattasio, F. Giorgi, F. Zuccarello, I. Ermolli, M. Stangalini, P. Romano","submitted_at":"2017-01-23T15:11:19Z","abstract_excerpt":"We studied the formation of a pore in AR NOAA 11462. We analysed data obtained with the IBIS at the DST on April 17, 2012, consisting of full Stokes measurements of the Fe I 617.3 nm lines. Furthermore, we analysed SDO/HMI observations in the continuum and vector magnetograms derived from the Fe I 617.3 nm line data taken from April 15 to 19, 2012. We estimated the magnetic field strength and vector components and the LOS and horizontal motions in the photospheric region hosting the pore formation. We discuss our results in light of other observational studies and recent advances of numerical "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.06440","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":"1701.06440","created_at":"2026-05-18T00:52:18.375043+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.06440v1","created_at":"2026-05-18T00:52:18.375043+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.06440","created_at":"2026-05-18T00:52:18.375043+00:00"},{"alias_kind":"pith_short_12","alias_value":"R2NUEJO52C2J","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_16","alias_value":"R2NUEJO52C2JTD4B","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_8","alias_value":"R2NUEJO5","created_at":"2026-05-18T12:31:39.905425+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/R2NUEJO52C2JTD4BLMCVISDGCN","json":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN.json","graph_json":"https://pith.science/api/pith-number/R2NUEJO52C2JTD4BLMCVISDGCN/graph.json","events_json":"https://pith.science/api/pith-number/R2NUEJO52C2JTD4BLMCVISDGCN/events.json","paper":"https://pith.science/paper/R2NUEJO5"},"agent_actions":{"view_html":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN","download_json":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN.json","view_paper":"https://pith.science/paper/R2NUEJO5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.06440&json=true","fetch_graph":"https://pith.science/api/pith-number/R2NUEJO52C2JTD4BLMCVISDGCN/graph.json","fetch_events":"https://pith.science/api/pith-number/R2NUEJO52C2JTD4BLMCVISDGCN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN/action/storage_attestation","attest_author":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN/action/author_attestation","sign_citation":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN/action/citation_signature","submit_replication":"https://pith.science/pith/R2NUEJO52C2JTD4BLMCVISDGCN/action/replication_record"}},"created_at":"2026-05-18T00:52:18.375043+00:00","updated_at":"2026-05-18T00:52:18.375043+00:00"}