{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:LKIUMEOPNWVR4UG35Y7XNZ6Q4N","short_pith_number":"pith:LKIUMEOP","schema_version":"1.0","canonical_sha256":"5a914611cf6dab1e50dbee3f76e7d0e34721dc75f2d74dc8bb7b2edbb786d350","source":{"kind":"arxiv","id":"1711.01508","version":2},"attestation_state":"computed","paper":{"title":"Nature of stochastic ion heating in the solar wind: testing the dependence on plasma beta and turbulence amplitude","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"physics.space-ph","authors_text":"Daniel Vech, Justin C. Kasper, Kristopher G. Klein","submitted_at":"2017-11-05T00:09:23Z","abstract_excerpt":"The solar wind undergoes significant heating as it propagates away from the Sun; the exact mechanisms responsible for this heating are not yet fully understood. We present for the first time a statistical test for one of the proposed mechanisms, stochastic ion heating. We use the amplitude of magnetic field fluctuations near the proton gyroscale as a proxy for the ratio of gyroscale velocity fluctuations to perpendicular (with respect to the magnetic field) proton thermal speed, defined as $\\epsilon_p$. Enhanced proton temperatures are observed when $\\epsilon_p$ is larger than a critical value"},"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":"1711.01508","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2017-11-05T00:09:23Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"d29dfd00a505f8e34ac84f89ed1a7dc3056dd9d4d69f69411cc65d4c2b02c24c","abstract_canon_sha256":"5e8d7359f8371095714b2793541a57598535aa94c0f6907eb5afb1881a7baebc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:29:24.424006Z","signature_b64":"CNNza9zIv49KlqwdDlRRxRtSemkGLNK1tEUbHaXkJ4bEA/IXH6ZBLHrENuMqKMaNusSS8jD5W4gFoXAG1JpdAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5a914611cf6dab1e50dbee3f76e7d0e34721dc75f2d74dc8bb7b2edbb786d350","last_reissued_at":"2026-05-18T00:29:24.423250Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:29:24.423250Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nature of stochastic ion heating in the solar wind: testing the dependence on plasma beta and turbulence amplitude","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"physics.space-ph","authors_text":"Daniel Vech, Justin C. Kasper, Kristopher G. Klein","submitted_at":"2017-11-05T00:09:23Z","abstract_excerpt":"The solar wind undergoes significant heating as it propagates away from the Sun; the exact mechanisms responsible for this heating are not yet fully understood. We present for the first time a statistical test for one of the proposed mechanisms, stochastic ion heating. We use the amplitude of magnetic field fluctuations near the proton gyroscale as a proxy for the ratio of gyroscale velocity fluctuations to perpendicular (with respect to the magnetic field) proton thermal speed, defined as $\\epsilon_p$. Enhanced proton temperatures are observed when $\\epsilon_p$ is larger than a critical value"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.01508","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":""},"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":"1711.01508","created_at":"2026-05-18T00:29:24.423391+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.01508v2","created_at":"2026-05-18T00:29:24.423391+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.01508","created_at":"2026-05-18T00:29:24.423391+00:00"},{"alias_kind":"pith_short_12","alias_value":"LKIUMEOPNWVR","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"LKIUMEOPNWVR4UG3","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"LKIUMEOP","created_at":"2026-05-18T12:31:28.150371+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/LKIUMEOPNWVR4UG35Y7XNZ6Q4N","json":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N.json","graph_json":"https://pith.science/api/pith-number/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/graph.json","events_json":"https://pith.science/api/pith-number/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/events.json","paper":"https://pith.science/paper/LKIUMEOP"},"agent_actions":{"view_html":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N","download_json":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N.json","view_paper":"https://pith.science/paper/LKIUMEOP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.01508&json=true","fetch_graph":"https://pith.science/api/pith-number/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/graph.json","fetch_events":"https://pith.science/api/pith-number/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/action/storage_attestation","attest_author":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/action/author_attestation","sign_citation":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/action/citation_signature","submit_replication":"https://pith.science/pith/LKIUMEOPNWVR4UG35Y7XNZ6Q4N/action/replication_record"}},"created_at":"2026-05-18T00:29:24.423391+00:00","updated_at":"2026-05-18T00:29:24.423391+00:00"}