{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:KYDHB5YLA4J5IMUBRZ7646ADX3","short_pith_number":"pith:KYDHB5YL","schema_version":"1.0","canonical_sha256":"560670f70b0713d432818e7fee7803beff6a0dbd7c5c94d2f2475c6d93523569","source":{"kind":"arxiv","id":"2201.03148","version":1},"attestation_state":"computed","paper":{"title":"Statistical Study on the Sources of Jovian Decametric Radio Emissions Based on the Radio Observations of Remote Instruments","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Chuanbing Wang, Ruobing Zheng, Xianzhe Jia, Xiaolei Li, Yuming Wang","submitted_at":"2022-01-10T03:24:41Z","abstract_excerpt":"To better understand the physical processes associated with Jovian decametric (DAM) radio emissions, we present the statistical study of DAMs and inferred characteristics of DAM sources based on multi-view observation from Wind and STEREO spacecraft. The distribution of the apparent rotation speed of DAMs derived from multiple spacecraft suggests that the rotation speed of Io-related DAMs is in range of 0.15-0.6{\\Omega}_J and that of non-Io-DAMs is between 0.7-1.2{\\Omega}_J. Based on the method of Wang et al. (2020), we locate the sources of the DAMs and infer their emission angles and associa"},"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":"2201.03148","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2022-01-10T03:24:41Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"08313867a1d0a1f25f50cb3c583026ba4c1e4d7f73df102672c3d937fe46e99c","abstract_canon_sha256":"95556bea74f347035f62a5b816190e25d14e256fc0a9a0997c74412f37328815"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:12:31.022502Z","signature_b64":"UOKR2AfGehjdc3qC1CQ5qRZZRU8LcgciF9HkRoXznEyIdlH0ASCikgQNGw+ZcmQriuZvEPq0ix0LNdRab1SMAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"560670f70b0713d432818e7fee7803beff6a0dbd7c5c94d2f2475c6d93523569","last_reissued_at":"2026-07-05T06:12:31.021953Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:12:31.021953Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Statistical Study on the Sources of Jovian Decametric Radio Emissions Based on the Radio Observations of Remote Instruments","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.EP","authors_text":"Chuanbing Wang, Ruobing Zheng, Xianzhe Jia, Xiaolei Li, Yuming Wang","submitted_at":"2022-01-10T03:24:41Z","abstract_excerpt":"To better understand the physical processes associated with Jovian decametric (DAM) radio emissions, we present the statistical study of DAMs and inferred characteristics of DAM sources based on multi-view observation from Wind and STEREO spacecraft. The distribution of the apparent rotation speed of DAMs derived from multiple spacecraft suggests that the rotation speed of Io-related DAMs is in range of 0.15-0.6{\\Omega}_J and that of non-Io-DAMs is between 0.7-1.2{\\Omega}_J. Based on the method of Wang et al. (2020), we locate the sources of the DAMs and infer their emission angles and associa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.03148","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/2201.03148/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":"2201.03148","created_at":"2026-07-05T06:12:31.022012+00:00"},{"alias_kind":"arxiv_version","alias_value":"2201.03148v1","created_at":"2026-07-05T06:12:31.022012+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2201.03148","created_at":"2026-07-05T06:12:31.022012+00:00"},{"alias_kind":"pith_short_12","alias_value":"KYDHB5YLA4J5","created_at":"2026-07-05T06:12:31.022012+00:00"},{"alias_kind":"pith_short_16","alias_value":"KYDHB5YLA4J5IMUB","created_at":"2026-07-05T06:12:31.022012+00:00"},{"alias_kind":"pith_short_8","alias_value":"KYDHB5YL","created_at":"2026-07-05T06:12:31.022012+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/KYDHB5YLA4J5IMUBRZ7646ADX3","json":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3.json","graph_json":"https://pith.science/api/pith-number/KYDHB5YLA4J5IMUBRZ7646ADX3/graph.json","events_json":"https://pith.science/api/pith-number/KYDHB5YLA4J5IMUBRZ7646ADX3/events.json","paper":"https://pith.science/paper/KYDHB5YL"},"agent_actions":{"view_html":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3","download_json":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3.json","view_paper":"https://pith.science/paper/KYDHB5YL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2201.03148&json=true","fetch_graph":"https://pith.science/api/pith-number/KYDHB5YLA4J5IMUBRZ7646ADX3/graph.json","fetch_events":"https://pith.science/api/pith-number/KYDHB5YLA4J5IMUBRZ7646ADX3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3/action/storage_attestation","attest_author":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3/action/author_attestation","sign_citation":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3/action/citation_signature","submit_replication":"https://pith.science/pith/KYDHB5YLA4J5IMUBRZ7646ADX3/action/replication_record"}},"created_at":"2026-07-05T06:12:31.022012+00:00","updated_at":"2026-07-05T06:12:31.022012+00:00"}