{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:GEP2RDBLMMV6KWP34ABCZT76TY","short_pith_number":"pith:GEP2RDBL","schema_version":"1.0","canonical_sha256":"311fa88c2b632be559fbe0022ccffe9e030e3174a47199b02255fc795438d134","source":{"kind":"arxiv","id":"1703.10140","version":1},"attestation_state":"computed","paper":{"title":"High-resolution imaging spectroscopy of two micro-pores and an arch filament system in a small emerging-flux region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Denker, N. Bello Gonz\\'alez, S. J. Gonz\\'alez Manrique","submitted_at":"2017-03-29T17:08:24Z","abstract_excerpt":"Aims. The purpose of this investigation is to characterize the temporal evolution of an emerging flux region, the associated photospheric and chromospheric flow fields, and the properties of the accompanying arch filament system. Methods. This study is based on imaging spectroscopy with the G\\\"ottingen Fabry-P\\'erot Interferometer at the Vacuum Tower Telescope, on 2008 August 7. Cloud model (CM) inversions of line scans in the strong chromospheric absorption H$\\alpha$ line yielded CM parameters, which describe the cool plasma contained in the arch filament system. Results. The observations cov"},"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":"1703.10140","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-03-29T17:08:24Z","cross_cats_sorted":[],"title_canon_sha256":"452ee98d53c06d53647ccb3084d3757d80d6e23a8968c962c68383c22e6b5b8b","abstract_canon_sha256":"3a09139ac3d3555c223992bcb11a918d79a67c8357c9fcbc18cd2b9d6affb51e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:47:38.573511Z","signature_b64":"5CLOQxMz9eupg4ZNmda8CIDL/dpmp38tiCm5nOLr5ZjqUiUNfR8bdACM6W+QFDmp7kqbasBQFZ1+r0KhvAy4Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"311fa88c2b632be559fbe0022ccffe9e030e3174a47199b02255fc795438d134","last_reissued_at":"2026-05-18T00:47:38.573009Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:47:38.573009Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-resolution imaging spectroscopy of two micro-pores and an arch filament system in a small emerging-flux region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Denker, N. Bello Gonz\\'alez, S. J. Gonz\\'alez Manrique","submitted_at":"2017-03-29T17:08:24Z","abstract_excerpt":"Aims. The purpose of this investigation is to characterize the temporal evolution of an emerging flux region, the associated photospheric and chromospheric flow fields, and the properties of the accompanying arch filament system. Methods. This study is based on imaging spectroscopy with the G\\\"ottingen Fabry-P\\'erot Interferometer at the Vacuum Tower Telescope, on 2008 August 7. Cloud model (CM) inversions of line scans in the strong chromospheric absorption H$\\alpha$ line yielded CM parameters, which describe the cool plasma contained in the arch filament system. Results. The observations cov"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.10140","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":"1703.10140","created_at":"2026-05-18T00:47:38.573095+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.10140v1","created_at":"2026-05-18T00:47:38.573095+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.10140","created_at":"2026-05-18T00:47:38.573095+00:00"},{"alias_kind":"pith_short_12","alias_value":"GEP2RDBLMMV6","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"GEP2RDBLMMV6KWP3","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"GEP2RDBL","created_at":"2026-05-18T12:31:15.632608+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/GEP2RDBLMMV6KWP34ABCZT76TY","json":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY.json","graph_json":"https://pith.science/api/pith-number/GEP2RDBLMMV6KWP34ABCZT76TY/graph.json","events_json":"https://pith.science/api/pith-number/GEP2RDBLMMV6KWP34ABCZT76TY/events.json","paper":"https://pith.science/paper/GEP2RDBL"},"agent_actions":{"view_html":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY","download_json":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY.json","view_paper":"https://pith.science/paper/GEP2RDBL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.10140&json=true","fetch_graph":"https://pith.science/api/pith-number/GEP2RDBLMMV6KWP34ABCZT76TY/graph.json","fetch_events":"https://pith.science/api/pith-number/GEP2RDBLMMV6KWP34ABCZT76TY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY/action/storage_attestation","attest_author":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY/action/author_attestation","sign_citation":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY/action/citation_signature","submit_replication":"https://pith.science/pith/GEP2RDBLMMV6KWP34ABCZT76TY/action/replication_record"}},"created_at":"2026-05-18T00:47:38.573095+00:00","updated_at":"2026-05-18T00:47:38.573095+00:00"}