{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:RW2ZPOFXD5CIJU54T5QRSAD4VL","short_pith_number":"pith:RW2ZPOFX","schema_version":"1.0","canonical_sha256":"8db597b8b71f4484d3bc9f6119007caae0e1bb0561a2c4aaefd0ac5dcbca4df1","source":{"kind":"arxiv","id":"1409.1118","version":1},"attestation_state":"computed","paper":{"title":"Extraordinary Solar Modulation Effects On Galactic Cosmic Rays Observed By V1 Near The Heliopause","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"J. J. Quenby, W. R. Webber","submitted_at":"2014-09-03T15:07:05Z","abstract_excerpt":"We discuss two extraordinary increases of cosmic ray intensity observed by Voyager 1 in the last 1.1 AU before heliopause crossing, Aug 2012 at 121.7 AU. The two increases are roughly similar in amplitude and result in a total increase of cosmic ray nuclei around 1 GV of over 50 percent and of 0.01 GV electrons of a factor about 2. During the first increase, the changes in the magnetic, B, field are small. After the first increase, the B field variations and cosmic ray changes become large and during the second increase the B field variations and the cosmic ray changes are correlated to within"},"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":"1409.1118","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-09-03T15:07:05Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"af243bd7eed5eb4c33fe2812ddd383d574d283ee631d77ed26652416af890d28","abstract_canon_sha256":"241ef2f2a8ca1765f9db1f13a526d145bb4d7ec42d038176e5632b777f953941"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:43:44.310467Z","signature_b64":"l9zvwYuM0unZGUXz/vtQCYT/V18SCfZXCG34fREMnrT6xVKFP4oXZP1V/dblOoSvWHGV1AGh9lpHsCCSHTTRAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8db597b8b71f4484d3bc9f6119007caae0e1bb0561a2c4aaefd0ac5dcbca4df1","last_reissued_at":"2026-05-18T02:43:44.309939Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:43:44.309939Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Extraordinary Solar Modulation Effects On Galactic Cosmic Rays Observed By V1 Near The Heliopause","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"J. J. Quenby, W. R. Webber","submitted_at":"2014-09-03T15:07:05Z","abstract_excerpt":"We discuss two extraordinary increases of cosmic ray intensity observed by Voyager 1 in the last 1.1 AU before heliopause crossing, Aug 2012 at 121.7 AU. The two increases are roughly similar in amplitude and result in a total increase of cosmic ray nuclei around 1 GV of over 50 percent and of 0.01 GV electrons of a factor about 2. During the first increase, the changes in the magnetic, B, field are small. After the first increase, the B field variations and cosmic ray changes become large and during the second increase the B field variations and the cosmic ray changes are correlated to within"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.1118","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":""},"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":"1409.1118","created_at":"2026-05-18T02:43:44.310007+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.1118v1","created_at":"2026-05-18T02:43:44.310007+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.1118","created_at":"2026-05-18T02:43:44.310007+00:00"},{"alias_kind":"pith_short_12","alias_value":"RW2ZPOFXD5CI","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"RW2ZPOFXD5CIJU54","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"RW2ZPOFX","created_at":"2026-05-18T12:28:46.137349+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/RW2ZPOFXD5CIJU54T5QRSAD4VL","json":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL.json","graph_json":"https://pith.science/api/pith-number/RW2ZPOFXD5CIJU54T5QRSAD4VL/graph.json","events_json":"https://pith.science/api/pith-number/RW2ZPOFXD5CIJU54T5QRSAD4VL/events.json","paper":"https://pith.science/paper/RW2ZPOFX"},"agent_actions":{"view_html":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL","download_json":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL.json","view_paper":"https://pith.science/paper/RW2ZPOFX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.1118&json=true","fetch_graph":"https://pith.science/api/pith-number/RW2ZPOFXD5CIJU54T5QRSAD4VL/graph.json","fetch_events":"https://pith.science/api/pith-number/RW2ZPOFXD5CIJU54T5QRSAD4VL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL/action/storage_attestation","attest_author":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL/action/author_attestation","sign_citation":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL/action/citation_signature","submit_replication":"https://pith.science/pith/RW2ZPOFXD5CIJU54T5QRSAD4VL/action/replication_record"}},"created_at":"2026-05-18T02:43:44.310007+00:00","updated_at":"2026-05-18T02:43:44.310007+00:00"}