{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:5XIPAMCQZZSK2MNWKGD7M6FA3W","short_pith_number":"pith:5XIPAMCQ","schema_version":"1.0","canonical_sha256":"edd0f03050ce64ad31b65187f678a0dd8542bb1ce1d747a25b1dda780bb70635","source":{"kind":"arxiv","id":"1708.06505","version":3},"attestation_state":"computed","paper":{"title":"Imaging Spectroscopy of Solar Radio Burst Fine Structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.plasm-ph","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"A. A. Kuznetsov, A. G. Emslie, B. Alcock, E. P. Kontar, N. H. Bian, N. L. S. Jeffrey, P. Subramanian, S. Yu, V. N. Melnik","submitted_at":"2017-08-22T06:11:44Z","abstract_excerpt":"Solar radio observations provide a unique diagnostic of the outer solar atmosphere. However, the inhomogeneous turbulent corona strongly affects the propagation of the emitted radio waves, so decoupling the intrinsic properties of the emitting source from the effects of radio-wave propagation has long been a major challenge in solar physics. Here we report quantitative spatial and frequency characterization of solar radio burst fine structures observed with the LOw Frequency Array (LOFAR), an instrument with high time resolution that also permits imaging at scales much shorter than those corre"},"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":"1708.06505","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-22T06:11:44Z","cross_cats_sorted":["astro-ph.HE","physics.plasm-ph","physics.space-ph"],"title_canon_sha256":"d13a38c50512bdc7f6bc7bd96b19c1488ce2837205742c822d858deac144a2fb","abstract_canon_sha256":"63915612b7be1e93d384fe67d27aa86604b60f3fb48554f2a5426166de4fc385"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:52.681503Z","signature_b64":"LhmV3HzVCy7AO4rAmfzqkxNRoPxvL+orsS45lfeJ7ucJzg6yGsH8MXXTDvos2ed3ymL+Kwc4rJqLwHq9Sab+Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"edd0f03050ce64ad31b65187f678a0dd8542bb1ce1d747a25b1dda780bb70635","last_reissued_at":"2026-05-18T00:22:52.681128Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:52.681128Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Imaging Spectroscopy of Solar Radio Burst Fine Structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.plasm-ph","physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"A. A. Kuznetsov, A. G. Emslie, B. Alcock, E. P. Kontar, N. H. Bian, N. L. S. Jeffrey, P. Subramanian, S. Yu, V. N. Melnik","submitted_at":"2017-08-22T06:11:44Z","abstract_excerpt":"Solar radio observations provide a unique diagnostic of the outer solar atmosphere. However, the inhomogeneous turbulent corona strongly affects the propagation of the emitted radio waves, so decoupling the intrinsic properties of the emitting source from the effects of radio-wave propagation has long been a major challenge in solar physics. Here we report quantitative spatial and frequency characterization of solar radio burst fine structures observed with the LOw Frequency Array (LOFAR), an instrument with high time resolution that also permits imaging at scales much shorter than those corre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.06505","kind":"arxiv","version":3},"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":"1708.06505","created_at":"2026-05-18T00:22:52.681183+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.06505v3","created_at":"2026-05-18T00:22:52.681183+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.06505","created_at":"2026-05-18T00:22:52.681183+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/5XIPAMCQZZSK2MNWKGD7M6FA3W","json":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W.json","graph_json":"https://pith.science/api/pith-number/5XIPAMCQZZSK2MNWKGD7M6FA3W/graph.json","events_json":"https://pith.science/api/pith-number/5XIPAMCQZZSK2MNWKGD7M6FA3W/events.json","paper":"https://pith.science/paper/5XIPAMCQ"},"agent_actions":{"view_html":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W","download_json":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W.json","view_paper":"https://pith.science/paper/5XIPAMCQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.06505&json=true","fetch_graph":"https://pith.science/api/pith-number/5XIPAMCQZZSK2MNWKGD7M6FA3W/graph.json","fetch_events":"https://pith.science/api/pith-number/5XIPAMCQZZSK2MNWKGD7M6FA3W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W/action/storage_attestation","attest_author":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W/action/author_attestation","sign_citation":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W/action/citation_signature","submit_replication":"https://pith.science/pith/5XIPAMCQZZSK2MNWKGD7M6FA3W/action/replication_record"}},"created_at":"2026-05-18T00:22:52.681183+00:00","updated_at":"2026-05-18T00:22:52.681183+00:00"}