{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:LASRO376BFK4JMZK6X3G4QVCWU","short_pith_number":"pith:LASRO376","schema_version":"1.0","canonical_sha256":"5825176ffe0955c4b32af5f66e42a2b505093f2d119362b0bb3e7ecd8b908fd6","source":{"kind":"arxiv","id":"2606.05514","version":1},"attestation_state":"computed","paper":{"title":"Complex Analysis of Askaryan Radiation: UHECR Reconstruction with Askaryan Radio Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. Ibanez-Rodriguez, J. C. Hanson","submitted_at":"2026-06-03T23:40:56Z","abstract_excerpt":"Ultra-high energy cosmic rays (UHECR) can produce relativistic cascades that emit radio-frequency (RF) pulses in the 0.05-1 GHz bandwidth via two distinct effects: the geomagnetic effect, and the Askaryan effect. The geomagnetic effect occurs when the magnetic field of the Earth causes cascade charges to form a transverse current that radiates linearly polarized radiation aligned with the Lorentz force direction. The Askaryan effect is caused by the net negative charge excess in the cascade that radiates linearly polarized radiation along the Cherenkov cone. When UHECR cascades enter solid, RF"},"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":"2606.05514","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-06-03T23:40:56Z","cross_cats_sorted":[],"title_canon_sha256":"d763a833c4019d71cce85db4c4e82f46dfca2d5b74013df6a3bd94e11190eb03","abstract_canon_sha256":"ff1d411eed4d91d9b955bdfc685a6fe66cbfd2b547072d5d37dd06e22c6323cb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-05T01:14:53.370450Z","signature_b64":"o39MBqbZMTpgei67Xutazl9t+rRQJptGhIEWFDbggrYLWX9+C0pWM3eOZpW6W8/GILf8cd68g+dlLwXmqXEMBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5825176ffe0955c4b32af5f66e42a2b505093f2d119362b0bb3e7ecd8b908fd6","last_reissued_at":"2026-06-05T01:14:53.370004Z","signature_status":"signed_v1","first_computed_at":"2026-06-05T01:14:53.370004Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Complex Analysis of Askaryan Radiation: UHECR Reconstruction with Askaryan Radio Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. Ibanez-Rodriguez, J. C. Hanson","submitted_at":"2026-06-03T23:40:56Z","abstract_excerpt":"Ultra-high energy cosmic rays (UHECR) can produce relativistic cascades that emit radio-frequency (RF) pulses in the 0.05-1 GHz bandwidth via two distinct effects: the geomagnetic effect, and the Askaryan effect. The geomagnetic effect occurs when the magnetic field of the Earth causes cascade charges to form a transverse current that radiates linearly polarized radiation aligned with the Lorentz force direction. The Askaryan effect is caused by the net negative charge excess in the cascade that radiates linearly polarized radiation along the Cherenkov cone. When UHECR cascades enter solid, RF"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.05514","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2606.05514/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2606.05514","created_at":"2026-06-05T01:14:53.370073+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.05514v1","created_at":"2026-06-05T01:14:53.370073+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.05514","created_at":"2026-06-05T01:14:53.370073+00:00"},{"alias_kind":"pith_short_12","alias_value":"LASRO376BFK4","created_at":"2026-06-05T01:14:53.370073+00:00"},{"alias_kind":"pith_short_16","alias_value":"LASRO376BFK4JMZK","created_at":"2026-06-05T01:14:53.370073+00:00"},{"alias_kind":"pith_short_8","alias_value":"LASRO376","created_at":"2026-06-05T01:14:53.370073+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/LASRO376BFK4JMZK6X3G4QVCWU","json":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU.json","graph_json":"https://pith.science/api/pith-number/LASRO376BFK4JMZK6X3G4QVCWU/graph.json","events_json":"https://pith.science/api/pith-number/LASRO376BFK4JMZK6X3G4QVCWU/events.json","paper":"https://pith.science/paper/LASRO376"},"agent_actions":{"view_html":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU","download_json":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU.json","view_paper":"https://pith.science/paper/LASRO376","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.05514&json=true","fetch_graph":"https://pith.science/api/pith-number/LASRO376BFK4JMZK6X3G4QVCWU/graph.json","fetch_events":"https://pith.science/api/pith-number/LASRO376BFK4JMZK6X3G4QVCWU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU/action/storage_attestation","attest_author":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU/action/author_attestation","sign_citation":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU/action/citation_signature","submit_replication":"https://pith.science/pith/LASRO376BFK4JMZK6X3G4QVCWU/action/replication_record"}},"created_at":"2026-06-05T01:14:53.370073+00:00","updated_at":"2026-06-05T01:14:53.370073+00:00"}