{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:ILXU5DFZSMQCDKUJZ3M6QPUZ6J","short_pith_number":"pith:ILXU5DFZ","schema_version":"1.0","canonical_sha256":"42ef4e8cb9932021aa89ced9e83e99f2432f231b866351c66612851f0a68fda2","source":{"kind":"arxiv","id":"1605.07677","version":2},"attestation_state":"computed","paper":{"title":"Analysis of intermittency in submillimeter radio and hard X-Rays during the impulsive phase of a solar flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Guillermo Gim\\'enez de Castro, Jean-Pierre Raulin, Odilon M. Guimar\\~aes Jr, Paulo J. A. Sim\\~oes","submitted_at":"2016-05-24T22:35:59Z","abstract_excerpt":"We present an analysis of intermittent processes occurred during the impulsive phase of the flare SOL2012-03-13, using hard X-rays and submillimeter radio data. Intermittency is a key characteristic in turbulent plasmas and have been a analyzed recently for hard X-rays data only. Since in a typical flare the same accelerated electron population is believed to produce both hard X-rays and gyrosynchrotron, we compare both time profiles searching for intermittency signatures. For that we define a cross-wavelet power spectrum, that is used to obtain the Local Intermittency Measure or LIM. When gre"},"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":"1605.07677","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-05-24T22:35:59Z","cross_cats_sorted":[],"title_canon_sha256":"e059842ae97a491156301d4880388526c375331936f1ad5e0094e19e8bcf99fe","abstract_canon_sha256":"3dcb9b8b0d2c331503df28dc05c58fc49e7f9e94066d8fb30453e436a20c337c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:11.490763Z","signature_b64":"KkHxD19nQfqQdfRelau57nont4+NcqI8H4k0u2fOcQe2M1bwqWVa7pD7d7HR7HEqd6LonguI5fSIfnSjqBAyAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"42ef4e8cb9932021aa89ced9e83e99f2432f231b866351c66612851f0a68fda2","last_reissued_at":"2026-05-18T01:12:11.490146Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:11.490146Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Analysis of intermittency in submillimeter radio and hard X-Rays during the impulsive phase of a solar flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Guillermo Gim\\'enez de Castro, Jean-Pierre Raulin, Odilon M. Guimar\\~aes Jr, Paulo J. A. Sim\\~oes","submitted_at":"2016-05-24T22:35:59Z","abstract_excerpt":"We present an analysis of intermittent processes occurred during the impulsive phase of the flare SOL2012-03-13, using hard X-rays and submillimeter radio data. Intermittency is a key characteristic in turbulent plasmas and have been a analyzed recently for hard X-rays data only. Since in a typical flare the same accelerated electron population is believed to produce both hard X-rays and gyrosynchrotron, we compare both time profiles searching for intermittency signatures. For that we define a cross-wavelet power spectrum, that is used to obtain the Local Intermittency Measure or LIM. When gre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.07677","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":"1605.07677","created_at":"2026-05-18T01:12:11.490238+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.07677v2","created_at":"2026-05-18T01:12:11.490238+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.07677","created_at":"2026-05-18T01:12:11.490238+00:00"},{"alias_kind":"pith_short_12","alias_value":"ILXU5DFZSMQC","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_16","alias_value":"ILXU5DFZSMQCDKUJ","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_8","alias_value":"ILXU5DFZ","created_at":"2026-05-18T12:30:22.444734+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/ILXU5DFZSMQCDKUJZ3M6QPUZ6J","json":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J.json","graph_json":"https://pith.science/api/pith-number/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/graph.json","events_json":"https://pith.science/api/pith-number/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/events.json","paper":"https://pith.science/paper/ILXU5DFZ"},"agent_actions":{"view_html":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J","download_json":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J.json","view_paper":"https://pith.science/paper/ILXU5DFZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.07677&json=true","fetch_graph":"https://pith.science/api/pith-number/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/graph.json","fetch_events":"https://pith.science/api/pith-number/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/action/storage_attestation","attest_author":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/action/author_attestation","sign_citation":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/action/citation_signature","submit_replication":"https://pith.science/pith/ILXU5DFZSMQCDKUJZ3M6QPUZ6J/action/replication_record"}},"created_at":"2026-05-18T01:12:11.490238+00:00","updated_at":"2026-05-18T01:12:11.490238+00:00"}