{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:TMAARK2L35A3IIF6C4BXE652AP","short_pith_number":"pith:TMAARK2L","schema_version":"1.0","canonical_sha256":"9b0008ab4bdf41b420be1703727bba03caf3d6b5ab26a1532e9d19b75954ef30","source":{"kind":"arxiv","id":"1207.1569","version":1},"attestation_state":"computed","paper":{"title":"The stellar scintillation on large and extremely large telescopes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Victor Kornilov","submitted_at":"2012-07-06T09:57:17Z","abstract_excerpt":"The accuracy of ground-based astronomical photometry is limited by two factors: photon statistics and stellar scintillation arising when star light passes through Earth's atmosphere. This paper examines the theoretical role of the outer scale $L_0$ of the optical turbulence (OT) which suppresses the low-frequency component of scintillation. It is shown that for typical values of $L_0 \\sim 25 - 50$ m, this effect becomes noticeable for a telescopes of diameter around 4 m. On extremely large, $30 - 40$ m, telescopes with exposures longer than a few seconds, the inclusion of the outer scale in th"},"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":"1207.1569","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2012-07-06T09:57:17Z","cross_cats_sorted":[],"title_canon_sha256":"64774036f378c4a941d62f083a6aa32f9071be3550a123e1174e5da6d259da83","abstract_canon_sha256":"84ce33dc4149d0dee028a53e8a17c2bbc87f13808076cdc4a480f40c24284173"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:33.853975Z","signature_b64":"/QMQxNFE3Y0ziMTvldiDVMFBGjwTq3PrXtV7ih8os5se+kbo3oxkWk85ySoF7aVa9U+Yqf4ZxwbNeUh3in5hBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b0008ab4bdf41b420be1703727bba03caf3d6b5ab26a1532e9d19b75954ef30","last_reissued_at":"2026-05-18T01:56:33.853420Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:33.853420Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The stellar scintillation on large and extremely large telescopes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Victor Kornilov","submitted_at":"2012-07-06T09:57:17Z","abstract_excerpt":"The accuracy of ground-based astronomical photometry is limited by two factors: photon statistics and stellar scintillation arising when star light passes through Earth's atmosphere. This paper examines the theoretical role of the outer scale $L_0$ of the optical turbulence (OT) which suppresses the low-frequency component of scintillation. It is shown that for typical values of $L_0 \\sim 25 - 50$ m, this effect becomes noticeable for a telescopes of diameter around 4 m. On extremely large, $30 - 40$ m, telescopes with exposures longer than a few seconds, the inclusion of the outer scale in th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.1569","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":"1207.1569","created_at":"2026-05-18T01:56:33.853521+00:00"},{"alias_kind":"arxiv_version","alias_value":"1207.1569v1","created_at":"2026-05-18T01:56:33.853521+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.1569","created_at":"2026-05-18T01:56:33.853521+00:00"},{"alias_kind":"pith_short_12","alias_value":"TMAARK2L35A3","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"TMAARK2L35A3IIF6","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"TMAARK2L","created_at":"2026-05-18T12:27:23.164592+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/TMAARK2L35A3IIF6C4BXE652AP","json":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP.json","graph_json":"https://pith.science/api/pith-number/TMAARK2L35A3IIF6C4BXE652AP/graph.json","events_json":"https://pith.science/api/pith-number/TMAARK2L35A3IIF6C4BXE652AP/events.json","paper":"https://pith.science/paper/TMAARK2L"},"agent_actions":{"view_html":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP","download_json":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP.json","view_paper":"https://pith.science/paper/TMAARK2L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1207.1569&json=true","fetch_graph":"https://pith.science/api/pith-number/TMAARK2L35A3IIF6C4BXE652AP/graph.json","fetch_events":"https://pith.science/api/pith-number/TMAARK2L35A3IIF6C4BXE652AP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP/action/storage_attestation","attest_author":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP/action/author_attestation","sign_citation":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP/action/citation_signature","submit_replication":"https://pith.science/pith/TMAARK2L35A3IIF6C4BXE652AP/action/replication_record"}},"created_at":"2026-05-18T01:56:33.853521+00:00","updated_at":"2026-05-18T01:56:33.853521+00:00"}