{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:TCRPBFAKYYTV7QPYE4UZY44R5X","short_pith_number":"pith:TCRPBFAK","schema_version":"1.0","canonical_sha256":"98a2f0940ac6275fc1f827299c7391edda74bef367828b91e478fd3d6d0f7bf8","source":{"kind":"arxiv","id":"1306.5336","version":1},"attestation_state":"computed","paper":{"title":"Solar Wind Turbulence and the Role of Ion Instabilities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Christopher H. K. Chen, Luca Sorriso-Valvo, Olga Alexandrova, Stuart D. Bale, Timothy S. Horbury","submitted_at":"2013-06-22T16:56:40Z","abstract_excerpt":"Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In addition to the presence of magnetic field, the differences with neutral fluid isotropic turbulence are: weakness of collisional dissipation and presence of several characteristic space and time scales. In this paper we discuss observational properties of solar wind turbulence in a large range from the MHD to the electron scales. At MHD scales, within the inertial range, turbulence cascade of magnetic fluctuations develops mostly in the plane perpendicular to the mean field. Solar wind turbulence is com"},"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":"1306.5336","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-06-22T16:56:40Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"3b047a2bc9085d0e179e7ec6f29b8c9d847df84a0ffd5e60a37a1130695db400","abstract_canon_sha256":"43fa441c083c4e29d5e3989573848026ef18f3eb78f4a7b3a9b37249f8bcf7ff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:13.676191Z","signature_b64":"NU2v0fsR4oCC5BcdZxPCLdAHvvnrsKs3jH7Phc2WYnjZ73BjEojvQUywWX6s0q5llOcSYGVW6VLTBZDlMeduDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98a2f0940ac6275fc1f827299c7391edda74bef367828b91e478fd3d6d0f7bf8","last_reissued_at":"2026-05-18T01:49:13.675653Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:13.675653Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar Wind Turbulence and the Role of Ion Instabilities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Christopher H. K. Chen, Luca Sorriso-Valvo, Olga Alexandrova, Stuart D. Bale, Timothy S. Horbury","submitted_at":"2013-06-22T16:56:40Z","abstract_excerpt":"Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In addition to the presence of magnetic field, the differences with neutral fluid isotropic turbulence are: weakness of collisional dissipation and presence of several characteristic space and time scales. In this paper we discuss observational properties of solar wind turbulence in a large range from the MHD to the electron scales. At MHD scales, within the inertial range, turbulence cascade of magnetic fluctuations develops mostly in the plane perpendicular to the mean field. Solar wind turbulence is com"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.5336","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":"1306.5336","created_at":"2026-05-18T01:49:13.675746+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.5336v1","created_at":"2026-05-18T01:49:13.675746+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.5336","created_at":"2026-05-18T01:49:13.675746+00:00"},{"alias_kind":"pith_short_12","alias_value":"TCRPBFAKYYTV","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"TCRPBFAKYYTV7QPY","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"TCRPBFAK","created_at":"2026-05-18T12:27:59.945178+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/TCRPBFAKYYTV7QPYE4UZY44R5X","json":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X.json","graph_json":"https://pith.science/api/pith-number/TCRPBFAKYYTV7QPYE4UZY44R5X/graph.json","events_json":"https://pith.science/api/pith-number/TCRPBFAKYYTV7QPYE4UZY44R5X/events.json","paper":"https://pith.science/paper/TCRPBFAK"},"agent_actions":{"view_html":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X","download_json":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X.json","view_paper":"https://pith.science/paper/TCRPBFAK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.5336&json=true","fetch_graph":"https://pith.science/api/pith-number/TCRPBFAKYYTV7QPYE4UZY44R5X/graph.json","fetch_events":"https://pith.science/api/pith-number/TCRPBFAKYYTV7QPYE4UZY44R5X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X/action/storage_attestation","attest_author":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X/action/author_attestation","sign_citation":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X/action/citation_signature","submit_replication":"https://pith.science/pith/TCRPBFAKYYTV7QPYE4UZY44R5X/action/replication_record"}},"created_at":"2026-05-18T01:49:13.675746+00:00","updated_at":"2026-05-18T01:49:13.675746+00:00"}