{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:ZSJN5PQZ2ICV6IRPEV5GJ6C4U5","short_pith_number":"pith:ZSJN5PQZ","schema_version":"1.0","canonical_sha256":"cc92debe19d2055f222f257a64f85ca760e78faaf6cee8ef4e0d34a91878fc7f","source":{"kind":"arxiv","id":"2007.06822","version":1},"attestation_state":"computed","paper":{"title":"A 3D framework to explore the propagation effects in stars exhibiting electron cyclotron maser emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Barnali Das, Poonam Chandra, Surajit Mondal","submitted_at":"2020-07-14T05:16:49Z","abstract_excerpt":"Recently, coherent radio emission has been discovered from a number of hot magnetic stars, via the process of electron cyclotron maser emission (ECME). This emission, observed in the form of highly circularly polarized pulses, have interesting properties which contain information about the host star. One of the important properties of ECME is the frequency dependence of the pulse arrival time. This has been attributed to propagation effect by Trigilio et al. (2011), and could explain the sequence observed for CU Vir qualitatively (Lo et al. 2012). However no quantitative treatment exists for t"},"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":"2007.06822","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2020-07-14T05:16:49Z","cross_cats_sorted":[],"title_canon_sha256":"5bc5be492ce9567ceef884afed8b4cc60b1e00265455075f5a4c1a1056b2a206","abstract_canon_sha256":"435d2015c30aa3982aaa671ff19d2d80379b0ce39d29e47df06c2cee274eb5f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:18:23.553633Z","signature_b64":"FQCp4s15w/7UGuU76wsAxLdD3SxQCj+Ishev7nNqiBMvk3PlAEzZNmMhimH4WgQ3OdIxuWhl89caTVAK2c3qAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc92debe19d2055f222f257a64f85ca760e78faaf6cee8ef4e0d34a91878fc7f","last_reissued_at":"2026-07-05T01:18:23.553221Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:18:23.553221Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A 3D framework to explore the propagation effects in stars exhibiting electron cyclotron maser emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Barnali Das, Poonam Chandra, Surajit Mondal","submitted_at":"2020-07-14T05:16:49Z","abstract_excerpt":"Recently, coherent radio emission has been discovered from a number of hot magnetic stars, via the process of electron cyclotron maser emission (ECME). This emission, observed in the form of highly circularly polarized pulses, have interesting properties which contain information about the host star. One of the important properties of ECME is the frequency dependence of the pulse arrival time. This has been attributed to propagation effect by Trigilio et al. (2011), and could explain the sequence observed for CU Vir qualitatively (Lo et al. 2012). However no quantitative treatment exists for t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.06822","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/2007.06822/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":"2007.06822","created_at":"2026-07-05T01:18:23.553274+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.06822v1","created_at":"2026-07-05T01:18:23.553274+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.06822","created_at":"2026-07-05T01:18:23.553274+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZSJN5PQZ2ICV","created_at":"2026-07-05T01:18:23.553274+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZSJN5PQZ2ICV6IRP","created_at":"2026-07-05T01:18:23.553274+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZSJN5PQZ","created_at":"2026-07-05T01:18:23.553274+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/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5","json":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5.json","graph_json":"https://pith.science/api/pith-number/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/graph.json","events_json":"https://pith.science/api/pith-number/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/events.json","paper":"https://pith.science/paper/ZSJN5PQZ"},"agent_actions":{"view_html":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5","download_json":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5.json","view_paper":"https://pith.science/paper/ZSJN5PQZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.06822&json=true","fetch_graph":"https://pith.science/api/pith-number/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/graph.json","fetch_events":"https://pith.science/api/pith-number/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/action/storage_attestation","attest_author":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/action/author_attestation","sign_citation":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/action/citation_signature","submit_replication":"https://pith.science/pith/ZSJN5PQZ2ICV6IRPEV5GJ6C4U5/action/replication_record"}},"created_at":"2026-07-05T01:18:23.553274+00:00","updated_at":"2026-07-05T01:18:23.553274+00:00"}