{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:LAPPAV5YBPLTQTJYSFQ6JM322B","short_pith_number":"pith:LAPPAV5Y","schema_version":"1.0","canonical_sha256":"581ef057b80bd7384d389161e4b37ad06f98c2d7aa4dce361536c0f2386babc4","source":{"kind":"arxiv","id":"2506.05923","version":2},"attestation_state":"computed","paper":{"title":"Convection Anisotropies of Cosmic Rays in Highly Magnetized Plasma","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Siming Liu, Yiran Zhang","submitted_at":"2025-06-06T09:44:34Z","abstract_excerpt":"Recently, Zhang & Liu (2024) proposed a turbulent convection model for multiscale anisotropies of cosmic rays (CRs), with an assumption of isotropic diffusion such that the anisotropies are statistically isotropic. However, this assumption may be unrealistic for TeV CRs, whose observations have revealed the significance of the local interstellar background magnetic field. To meet the difficulty, the turbulent convection scenario needs to be extended to cover anisotropic diffusion. In this paper, we focus on the parallel diffusion with isotropic pitch-angle scattering, which may be an approxima"},"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":"2506.05923","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-06-06T09:44:34Z","cross_cats_sorted":[],"title_canon_sha256":"b483ade2b38e51857b42516a7bf14458873730629451682977594153e5ae8af0","abstract_canon_sha256":"f43399e30dfebdbfc2b007a1c7fbdf94dff6e799998d6ee29f969c97afdf595b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:26:52.366013Z","signature_b64":"kYSXloaBdkxCkYmZ7hE/FBR3T0sq7dFwDaPi2ano/zd+nMEW0SWmyPHLi+ftIj9WV2s0WkQhpldRssnoViy8AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"581ef057b80bd7384d389161e4b37ad06f98c2d7aa4dce361536c0f2386babc4","last_reissued_at":"2026-07-05T11:26:52.365492Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:26:52.365492Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Convection Anisotropies of Cosmic Rays in Highly Magnetized Plasma","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Siming Liu, Yiran Zhang","submitted_at":"2025-06-06T09:44:34Z","abstract_excerpt":"Recently, Zhang & Liu (2024) proposed a turbulent convection model for multiscale anisotropies of cosmic rays (CRs), with an assumption of isotropic diffusion such that the anisotropies are statistically isotropic. However, this assumption may be unrealistic for TeV CRs, whose observations have revealed the significance of the local interstellar background magnetic field. To meet the difficulty, the turbulent convection scenario needs to be extended to cover anisotropic diffusion. In this paper, we focus on the parallel diffusion with isotropic pitch-angle scattering, which may be an approxima"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.05923","kind":"arxiv","version":2},"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/2506.05923/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":"2506.05923","created_at":"2026-07-05T11:26:52.365560+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.05923v2","created_at":"2026-07-05T11:26:52.365560+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.05923","created_at":"2026-07-05T11:26:52.365560+00:00"},{"alias_kind":"pith_short_12","alias_value":"LAPPAV5YBPLT","created_at":"2026-07-05T11:26:52.365560+00:00"},{"alias_kind":"pith_short_16","alias_value":"LAPPAV5YBPLTQTJY","created_at":"2026-07-05T11:26:52.365560+00:00"},{"alias_kind":"pith_short_8","alias_value":"LAPPAV5Y","created_at":"2026-07-05T11:26:52.365560+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/LAPPAV5YBPLTQTJYSFQ6JM322B","json":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B.json","graph_json":"https://pith.science/api/pith-number/LAPPAV5YBPLTQTJYSFQ6JM322B/graph.json","events_json":"https://pith.science/api/pith-number/LAPPAV5YBPLTQTJYSFQ6JM322B/events.json","paper":"https://pith.science/paper/LAPPAV5Y"},"agent_actions":{"view_html":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B","download_json":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B.json","view_paper":"https://pith.science/paper/LAPPAV5Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.05923&json=true","fetch_graph":"https://pith.science/api/pith-number/LAPPAV5YBPLTQTJYSFQ6JM322B/graph.json","fetch_events":"https://pith.science/api/pith-number/LAPPAV5YBPLTQTJYSFQ6JM322B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B/action/storage_attestation","attest_author":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B/action/author_attestation","sign_citation":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B/action/citation_signature","submit_replication":"https://pith.science/pith/LAPPAV5YBPLTQTJYSFQ6JM322B/action/replication_record"}},"created_at":"2026-07-05T11:26:52.365560+00:00","updated_at":"2026-07-05T11:26:52.365560+00:00"}