{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:OCXOSUC77UM2PRNFOLKBXTUPID","short_pith_number":"pith:OCXOSUC7","schema_version":"1.0","canonical_sha256":"70aee9505ffd19a7c5a572d41bce8f40c03ca7637a54c1650de71853fed3359e","source":{"kind":"arxiv","id":"1308.4556","version":1},"attestation_state":"computed","paper":{"title":"Spectral evolution of two-dimensional kinetic plasma turbulence in the wavenumber-frequency domain","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"D. Verscharen, H. Comi\\c{s}el, U. Motschmann, Y. Narita","submitted_at":"2013-08-21T12:43:29Z","abstract_excerpt":"We present a method for studying the evolution of plasma turbulence by tracking dispersion relations in the energy spectrum in the wavenumber-frequency domain. We apply hybrid plasma simulations in a simplified two-dimensional geometry to demonstrate our method and its applicability to plasma turbulence in the ion kinetic regime. We identify four dispersion relations: ion-Bernstein waves, oblique whistler waves, oblique Alfv\\'en/ion-cyclotron waves, and a zero-frequency mode. The energy partition and frequency broadening are evaluated for these modes. The method allows us to determine the evol"},"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":"1308.4556","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2013-08-21T12:43:29Z","cross_cats_sorted":["astro-ph.SR","physics.space-ph"],"title_canon_sha256":"f2c189f374fb7a7100767f642b7b1935ee903d2e9aa4f2fc3aad94d73a36ec27","abstract_canon_sha256":"5f3feb92cc1d25f26912f1bf758ac523bb6204276aaf07b410eb9deb450fd367"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:12:59.594147Z","signature_b64":"mP3CDcUr8hbrqdHLMmEERYs+qAmg3gg7aOzmCxqvy69I5btNo0HIYX6fXs4JYez8OGABP/gr/uDuw9jwCx35Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"70aee9505ffd19a7c5a572d41bce8f40c03ca7637a54c1650de71853fed3359e","last_reissued_at":"2026-05-18T03:12:59.593346Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:12:59.593346Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectral evolution of two-dimensional kinetic plasma turbulence in the wavenumber-frequency domain","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"D. Verscharen, H. Comi\\c{s}el, U. Motschmann, Y. Narita","submitted_at":"2013-08-21T12:43:29Z","abstract_excerpt":"We present a method for studying the evolution of plasma turbulence by tracking dispersion relations in the energy spectrum in the wavenumber-frequency domain. We apply hybrid plasma simulations in a simplified two-dimensional geometry to demonstrate our method and its applicability to plasma turbulence in the ion kinetic regime. We identify four dispersion relations: ion-Bernstein waves, oblique whistler waves, oblique Alfv\\'en/ion-cyclotron waves, and a zero-frequency mode. The energy partition and frequency broadening are evaluated for these modes. The method allows us to determine the evol"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.4556","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":"1308.4556","created_at":"2026-05-18T03:12:59.593482+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.4556v1","created_at":"2026-05-18T03:12:59.593482+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.4556","created_at":"2026-05-18T03:12:59.593482+00:00"},{"alias_kind":"pith_short_12","alias_value":"OCXOSUC77UM2","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_16","alias_value":"OCXOSUC77UM2PRNF","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_8","alias_value":"OCXOSUC7","created_at":"2026-05-18T12:27:54.935989+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/OCXOSUC77UM2PRNFOLKBXTUPID","json":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID.json","graph_json":"https://pith.science/api/pith-number/OCXOSUC77UM2PRNFOLKBXTUPID/graph.json","events_json":"https://pith.science/api/pith-number/OCXOSUC77UM2PRNFOLKBXTUPID/events.json","paper":"https://pith.science/paper/OCXOSUC7"},"agent_actions":{"view_html":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID","download_json":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID.json","view_paper":"https://pith.science/paper/OCXOSUC7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.4556&json=true","fetch_graph":"https://pith.science/api/pith-number/OCXOSUC77UM2PRNFOLKBXTUPID/graph.json","fetch_events":"https://pith.science/api/pith-number/OCXOSUC77UM2PRNFOLKBXTUPID/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID/action/storage_attestation","attest_author":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID/action/author_attestation","sign_citation":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID/action/citation_signature","submit_replication":"https://pith.science/pith/OCXOSUC77UM2PRNFOLKBXTUPID/action/replication_record"}},"created_at":"2026-05-18T03:12:59.593482+00:00","updated_at":"2026-05-18T03:12:59.593482+00:00"}