{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:2JRPFDQAQUTIHVU4GMOLPUQ2BL","short_pith_number":"pith:2JRPFDQA","schema_version":"1.0","canonical_sha256":"d262f28e00852683d69c331cb7d21a0aeab1ed6b3d16fc622e350571b02941fc","source":{"kind":"arxiv","id":"1306.6093","version":2},"attestation_state":"computed","paper":{"title":"Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Beck, D. Fabbian, F. Moreno-Insertis, K.G. Puschmann, R. Rezaei","submitted_at":"2013-06-25T21:21:53Z","abstract_excerpt":"Numerical 3D radiative (M)HD simulations of solar convection are used to understand the physical properties of the solar photosphere. To validate this approach, it is important to check that no excessive thermodynamic fluctuations arise as a consequence of the partially incomplete treatment of radiative transfer. We investigate the realism of 3D convection simulations carried out with the Stagger code. We compared the characteristic properties of several spectral lines in solar disc centre observations with spectra synthesized from the simulations. We degraded the synthetic spectra to the spat"},"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":"1306.6093","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-06-25T21:21:53Z","cross_cats_sorted":[],"title_canon_sha256":"b7c3f0287c070b97eddca1abd4230bf3b238dd15dd85efbabfd2fd7cda0d7294","abstract_canon_sha256":"41583eaf3c00a491ea642e77249d96d9a3d082965dca49a70e2a5559b3ea592a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:07.849472Z","signature_b64":"J1dkxeGVQsF5RgpB5QMWI90FsYR0W5zx32488BTK+A76oM5ebalk21KkLrnn9qjnMN048HlFfrSjHmi3ytFvBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d262f28e00852683d69c331cb7d21a0aeab1ed6b3d16fc622e350571b02941fc","last_reissued_at":"2026-05-18T01:49:07.848813Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:07.848813Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Beck, D. Fabbian, F. Moreno-Insertis, K.G. Puschmann, R. Rezaei","submitted_at":"2013-06-25T21:21:53Z","abstract_excerpt":"Numerical 3D radiative (M)HD simulations of solar convection are used to understand the physical properties of the solar photosphere. To validate this approach, it is important to check that no excessive thermodynamic fluctuations arise as a consequence of the partially incomplete treatment of radiative transfer. We investigate the realism of 3D convection simulations carried out with the Stagger code. We compared the characteristic properties of several spectral lines in solar disc centre observations with spectra synthesized from the simulations. We degraded the synthetic spectra to the spat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.6093","kind":"arxiv","version":2},"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":"1306.6093","created_at":"2026-05-18T01:49:07.848907+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.6093v2","created_at":"2026-05-18T01:49:07.848907+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.6093","created_at":"2026-05-18T01:49:07.848907+00:00"},{"alias_kind":"pith_short_12","alias_value":"2JRPFDQAQUTI","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_16","alias_value":"2JRPFDQAQUTIHVU4","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_8","alias_value":"2JRPFDQA","created_at":"2026-05-18T12:27:30.460161+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/2JRPFDQAQUTIHVU4GMOLPUQ2BL","json":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL.json","graph_json":"https://pith.science/api/pith-number/2JRPFDQAQUTIHVU4GMOLPUQ2BL/graph.json","events_json":"https://pith.science/api/pith-number/2JRPFDQAQUTIHVU4GMOLPUQ2BL/events.json","paper":"https://pith.science/paper/2JRPFDQA"},"agent_actions":{"view_html":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL","download_json":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL.json","view_paper":"https://pith.science/paper/2JRPFDQA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.6093&json=true","fetch_graph":"https://pith.science/api/pith-number/2JRPFDQAQUTIHVU4GMOLPUQ2BL/graph.json","fetch_events":"https://pith.science/api/pith-number/2JRPFDQAQUTIHVU4GMOLPUQ2BL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL/action/storage_attestation","attest_author":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL/action/author_attestation","sign_citation":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL/action/citation_signature","submit_replication":"https://pith.science/pith/2JRPFDQAQUTIHVU4GMOLPUQ2BL/action/replication_record"}},"created_at":"2026-05-18T01:49:07.848907+00:00","updated_at":"2026-05-18T01:49:07.848907+00:00"}