{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:SH3ZSLY55UPPJM3BGU3OSL4OPT","short_pith_number":"pith:SH3ZSLY5","schema_version":"1.0","canonical_sha256":"91f7992f1ded1ef4b3613536e92f8e7cd3813625a64fee38c670400af3ea2952","source":{"kind":"arxiv","id":"0910.4449","version":1},"attestation_state":"computed","paper":{"title":"Magnetic loop emergence within a granule","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2) Instituto de Astrof\\'isica de Canarias (IAC), (3) Astrophysikalisches Institut Potsdam, 4), (4) Astronomical Institute, (5) Kiepenheuer-Institut f\\\"ur Sonnenphysik, A. Kucera (4), Austria, C. Beck (2), Freiburg, Germany, Germany), H. Balthasar (3), H. W\\\"ohl (5) ((1) IGAM/Kanzelh\\\"ohe Observatory, Institute of Physics, J. Koza (4), J. Ryb\\'ak (4), P. G\\\"om\\\"ory (1, Slovak Academy of Sciences, Slovakia, Spain, Tatransk\\'a Lomnica, Universit\\\"at Graz","submitted_at":"2009-10-23T14:17:33Z","abstract_excerpt":"We investigate the temporal evolution of magnetic flux emerging within a granule in the quiet-Sun internetwork at disk center. We combined IR spectropolarimetry performed in two Fe I lines at 1565 nm with speckle-reconstructed G-band imaging. We determined the magnetic field parameters by a LTE inversion of the full Stokes vector using the SIR code, and followed their evolution in time. To interpret the observations, we created a geometrical model of a rising loop in 3D. The relevant parameters of the loop were matched to the observations where possible. We then synthesized spectra from the 3D"},"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":"0910.4449","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2009-10-23T14:17:33Z","cross_cats_sorted":[],"title_canon_sha256":"afc048ed84aed39a490a5a19e5ba2e96cc7cb4ea995c815406f3f123e0697bfd","abstract_canon_sha256":"a9b01ac71a3db5f35978635a945d09106fc352262a42d8084a2eeaf233c13331"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:27:22.912402Z","signature_b64":"YiYkahWqpkR+hWLBLS6QQikLXMB3XB7wbmDcoKMOKTp8lhAqopJv0TIY/TQ4XWq9DUmkTADsajQBnteaKXzvDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"91f7992f1ded1ef4b3613536e92f8e7cd3813625a64fee38c670400af3ea2952","last_reissued_at":"2026-05-18T00:27:22.911788Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:27:22.911788Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Magnetic loop emergence within a granule","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2) Instituto de Astrof\\'isica de Canarias (IAC), (3) Astrophysikalisches Institut Potsdam, 4), (4) Astronomical Institute, (5) Kiepenheuer-Institut f\\\"ur Sonnenphysik, A. Kucera (4), Austria, C. Beck (2), Freiburg, Germany, Germany), H. Balthasar (3), H. W\\\"ohl (5) ((1) IGAM/Kanzelh\\\"ohe Observatory, Institute of Physics, J. Koza (4), J. Ryb\\'ak (4), P. G\\\"om\\\"ory (1, Slovak Academy of Sciences, Slovakia, Spain, Tatransk\\'a Lomnica, Universit\\\"at Graz","submitted_at":"2009-10-23T14:17:33Z","abstract_excerpt":"We investigate the temporal evolution of magnetic flux emerging within a granule in the quiet-Sun internetwork at disk center. We combined IR spectropolarimetry performed in two Fe I lines at 1565 nm with speckle-reconstructed G-band imaging. We determined the magnetic field parameters by a LTE inversion of the full Stokes vector using the SIR code, and followed their evolution in time. To interpret the observations, we created a geometrical model of a rising loop in 3D. The relevant parameters of the loop were matched to the observations where possible. We then synthesized spectra from the 3D"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0910.4449","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":"0910.4449","created_at":"2026-05-18T00:27:22.911896+00:00"},{"alias_kind":"arxiv_version","alias_value":"0910.4449v1","created_at":"2026-05-18T00:27:22.911896+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0910.4449","created_at":"2026-05-18T00:27:22.911896+00:00"},{"alias_kind":"pith_short_12","alias_value":"SH3ZSLY55UPP","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"SH3ZSLY55UPPJM3B","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"SH3ZSLY5","created_at":"2026-05-18T12:26:01.383474+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/SH3ZSLY55UPPJM3BGU3OSL4OPT","json":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT.json","graph_json":"https://pith.science/api/pith-number/SH3ZSLY55UPPJM3BGU3OSL4OPT/graph.json","events_json":"https://pith.science/api/pith-number/SH3ZSLY55UPPJM3BGU3OSL4OPT/events.json","paper":"https://pith.science/paper/SH3ZSLY5"},"agent_actions":{"view_html":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT","download_json":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT.json","view_paper":"https://pith.science/paper/SH3ZSLY5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0910.4449&json=true","fetch_graph":"https://pith.science/api/pith-number/SH3ZSLY55UPPJM3BGU3OSL4OPT/graph.json","fetch_events":"https://pith.science/api/pith-number/SH3ZSLY55UPPJM3BGU3OSL4OPT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT/action/storage_attestation","attest_author":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT/action/author_attestation","sign_citation":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT/action/citation_signature","submit_replication":"https://pith.science/pith/SH3ZSLY55UPPJM3BGU3OSL4OPT/action/replication_record"}},"created_at":"2026-05-18T00:27:22.911896+00:00","updated_at":"2026-05-18T00:27:22.911896+00:00"}