{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:5E3MIQUT3XW5N2RHGZNE7BWICY","short_pith_number":"pith:5E3MIQUT","schema_version":"1.0","canonical_sha256":"e936c44293ddedd6ea27365a4f86c8162624d965d7662746721406c2bba1687b","source":{"kind":"arxiv","id":"1512.01763","version":1},"attestation_state":"computed","paper":{"title":"Comparison of 30 THz impulsive burst time development to microwaves, H-alpha, EUV, and GOES soft X-rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Kerdraon, A. S. Kudaka, D. P. Cabezas, G. Trottet, J.-P. Raulin, L. O. T. Fernandes, M. Karlicky, M. L. Luoni, M. M. Cassiano, P. Kaufmann, R. Marcon, R. Miteva, S. L. Freeland, S. M. White","submitted_at":"2015-12-06T09:50:01Z","abstract_excerpt":"The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretation challenges. One event associated with a GOES M2 class flare has been observed simultaneously in microwaves, H-alpha, EUV, and soft X-ray bands. Although these new observations confirm some features found in the two prior known events, they exhibit time profile structure discrepancies between 30 THz, microwaves, and hard X-rays (as inferred from the Neupert effect). These results suggest a more complex relationship between 30 THz emission and radiation produced at other wavelength ranges. The"},"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":"1512.01763","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-12-06T09:50:01Z","cross_cats_sorted":[],"title_canon_sha256":"4202449a57c6f534a6c5a8186f96bcf388bdc3ed24482bca831aa1090857bd27","abstract_canon_sha256":"d21d49492771577b36b1d1030102da972613dc7252becf96677fec4b1b5c58f3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:21:26.174575Z","signature_b64":"PrxII/9OJawSQpUvsb4x/5DRSzT3yPGbXN8U1cf3koGT9auTo6L+DxAEJeh1j7OuaHbxFSJ2n3kKwCOb0vB6Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e936c44293ddedd6ea27365a4f86c8162624d965d7662746721406c2bba1687b","last_reissued_at":"2026-05-18T01:21:26.173849Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:21:26.173849Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comparison of 30 THz impulsive burst time development to microwaves, H-alpha, EUV, and GOES soft X-rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Kerdraon, A. S. Kudaka, D. P. Cabezas, G. Trottet, J.-P. Raulin, L. O. T. Fernandes, M. Karlicky, M. L. Luoni, M. M. Cassiano, P. Kaufmann, R. Marcon, R. Miteva, S. L. Freeland, S. M. White","submitted_at":"2015-12-06T09:50:01Z","abstract_excerpt":"The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretation challenges. One event associated with a GOES M2 class flare has been observed simultaneously in microwaves, H-alpha, EUV, and soft X-ray bands. Although these new observations confirm some features found in the two prior known events, they exhibit time profile structure discrepancies between 30 THz, microwaves, and hard X-rays (as inferred from the Neupert effect). These results suggest a more complex relationship between 30 THz emission and radiation produced at other wavelength ranges. The"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.01763","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":"1512.01763","created_at":"2026-05-18T01:21:26.173971+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.01763v1","created_at":"2026-05-18T01:21:26.173971+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.01763","created_at":"2026-05-18T01:21:26.173971+00:00"},{"alias_kind":"pith_short_12","alias_value":"5E3MIQUT3XW5","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_16","alias_value":"5E3MIQUT3XW5N2RH","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_8","alias_value":"5E3MIQUT","created_at":"2026-05-18T12:29:05.191682+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/5E3MIQUT3XW5N2RHGZNE7BWICY","json":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY.json","graph_json":"https://pith.science/api/pith-number/5E3MIQUT3XW5N2RHGZNE7BWICY/graph.json","events_json":"https://pith.science/api/pith-number/5E3MIQUT3XW5N2RHGZNE7BWICY/events.json","paper":"https://pith.science/paper/5E3MIQUT"},"agent_actions":{"view_html":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY","download_json":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY.json","view_paper":"https://pith.science/paper/5E3MIQUT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.01763&json=true","fetch_graph":"https://pith.science/api/pith-number/5E3MIQUT3XW5N2RHGZNE7BWICY/graph.json","fetch_events":"https://pith.science/api/pith-number/5E3MIQUT3XW5N2RHGZNE7BWICY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY/action/storage_attestation","attest_author":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY/action/author_attestation","sign_citation":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY/action/citation_signature","submit_replication":"https://pith.science/pith/5E3MIQUT3XW5N2RHGZNE7BWICY/action/replication_record"}},"created_at":"2026-05-18T01:21:26.173971+00:00","updated_at":"2026-05-18T01:21:26.173971+00:00"}