{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:4S2U26NVLCOKAE6ZQ5IGB2HDKL","short_pith_number":"pith:4S2U26NV","schema_version":"1.0","canonical_sha256":"e4b54d79b5589ca013d9875060e8e352e6b6a009d16d55450759d78c21c55647","source":{"kind":"arxiv","id":"astro-ph/0612389","version":1},"attestation_state":"computed","paper":{"title":"A near-IR line of Mn I as a diagnostic tool of the average magnetic energy in the solar photosphere","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) THEMIS, 3), (3) CSIC), A. Asensio Ramos (1), A. Lopez Ariste (2), J. Trujillo Bueno (1, M. Collados (1) ((1) IAC, M. J. Martinez Gonzalez (1)","submitted_at":"2006-12-14T16:34:36Z","abstract_excerpt":"We report on spectropolarimetric observations of a near-IR line of Mn I located at 15262.702 A whose intensity and polarization profiles are very sensitive to the presence of hyperfine structure. A theoretical investigation of the magnetic sensitivity of this line to the magnetic field uncovers several interesting properties. The most important one is that the presence of strong Paschen-Back perturbations due to the hyperfine structure produces an intensity line profile whose shape changes according to the absolute value of the magnetic field strength. A line ratio technique is developed from "},"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":"astro-ph/0612389","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-14T16:34:36Z","cross_cats_sorted":[],"title_canon_sha256":"c8c3704452c0626f0b21dfbfd89828f8eb5792763e8d0378a81f79c43a8995c0","abstract_canon_sha256":"7850f1abae99df08216bd1b3e61caa69b5268a29b0c4052b75dd7443ce2a95d9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:29:14.802665Z","signature_b64":"c8g+pwe9eS/43zEr/7TlRK4hvK9GulS3UDiakMddh7F9ZIMuNrEGyO4EZs0ZPkOoOhKG3KaWeJvNyQM4HT2hDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e4b54d79b5589ca013d9875060e8e352e6b6a009d16d55450759d78c21c55647","last_reissued_at":"2026-05-18T04:29:14.801639Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:29:14.801639Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A near-IR line of Mn I as a diagnostic tool of the average magnetic energy in the solar photosphere","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) THEMIS, 3), (3) CSIC), A. Asensio Ramos (1), A. Lopez Ariste (2), J. Trujillo Bueno (1, M. Collados (1) ((1) IAC, M. J. Martinez Gonzalez (1)","submitted_at":"2006-12-14T16:34:36Z","abstract_excerpt":"We report on spectropolarimetric observations of a near-IR line of Mn I located at 15262.702 A whose intensity and polarization profiles are very sensitive to the presence of hyperfine structure. A theoretical investigation of the magnetic sensitivity of this line to the magnetic field uncovers several interesting properties. The most important one is that the presence of strong Paschen-Back perturbations due to the hyperfine structure produces an intensity line profile whose shape changes according to the absolute value of the magnetic field strength. A line ratio technique is developed from "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612389","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":"astro-ph/0612389","created_at":"2026-05-18T04:29:14.801779+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0612389v1","created_at":"2026-05-18T04:29:14.801779+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0612389","created_at":"2026-05-18T04:29:14.801779+00:00"},{"alias_kind":"pith_short_12","alias_value":"4S2U26NVLCOK","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"4S2U26NVLCOKAE6Z","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"4S2U26NV","created_at":"2026-05-18T12:25:53.939244+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/4S2U26NVLCOKAE6ZQ5IGB2HDKL","json":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL.json","graph_json":"https://pith.science/api/pith-number/4S2U26NVLCOKAE6ZQ5IGB2HDKL/graph.json","events_json":"https://pith.science/api/pith-number/4S2U26NVLCOKAE6ZQ5IGB2HDKL/events.json","paper":"https://pith.science/paper/4S2U26NV"},"agent_actions":{"view_html":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL","download_json":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL.json","view_paper":"https://pith.science/paper/4S2U26NV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0612389&json=true","fetch_graph":"https://pith.science/api/pith-number/4S2U26NVLCOKAE6ZQ5IGB2HDKL/graph.json","fetch_events":"https://pith.science/api/pith-number/4S2U26NVLCOKAE6ZQ5IGB2HDKL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL/action/storage_attestation","attest_author":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL/action/author_attestation","sign_citation":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL/action/citation_signature","submit_replication":"https://pith.science/pith/4S2U26NVLCOKAE6ZQ5IGB2HDKL/action/replication_record"}},"created_at":"2026-05-18T04:29:14.801779+00:00","updated_at":"2026-05-18T04:29:14.801779+00:00"}