{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:YAACHAFCPGRQTL3MCISMYBSBBE","short_pith_number":"pith:YAACHAFC","schema_version":"1.0","canonical_sha256":"c0002380a279a309af6c1224cc0641090c3ccc19d9ed1d6fbeae8e78e47ca702","source":{"kind":"arxiv","id":"1201.2784","version":2},"attestation_state":"computed","paper":{"title":"Kinetic cascade beyond magnetohydrodynamics of solar wind turbulence in two-dimensional hybrid simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Daniel Verscharen, Eckart Marsch, Joachim M\\\"uller, Uwe Motschmann","submitted_at":"2012-01-13T10:01:01Z","abstract_excerpt":"The nature of solar wind turbulence in the dissipation range at scales much smaller than the large MHD scales remains under debate. Here a two-dimensional model based on the hybrid code abbreviated as A.I.K.E.F. is presented, which treats massive ions as particles obeying the kinetic Vlasov equation and massless electrons as a neutralizing fluid. Up to a certain wavenumber in the MHD regime, the numerical system is initialized by assuming a superposition of isotropic Alfv\\'en waves with amplitudes that follow the empirically confirmed spectral law of Kolmogorov. Then turbulence develops and en"},"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":"1201.2784","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2012-01-13T10:01:01Z","cross_cats_sorted":["astro-ph.SR","physics.plasm-ph"],"title_canon_sha256":"d8fdc07af9ea33bfd950d4608bc37e84ac29be50a62552855ad1f7028491028c","abstract_canon_sha256":"f88c443c5ca8d3bb9e3146ba1d3c11be1b19b175984f46210b92c2defe691000"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:02:03.623709Z","signature_b64":"jNZ2F5xWlssai0FP8Rk4oDlBQ/6Ia6aUtuYg9/Eqtvyir1Y5yNabi73uuE6dubrp7sJSx0/YCWtzFlwrXAMUAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c0002380a279a309af6c1224cc0641090c3ccc19d9ed1d6fbeae8e78e47ca702","last_reissued_at":"2026-05-18T04:02:03.623231Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:02:03.623231Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinetic cascade beyond magnetohydrodynamics of solar wind turbulence in two-dimensional hybrid simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Daniel Verscharen, Eckart Marsch, Joachim M\\\"uller, Uwe Motschmann","submitted_at":"2012-01-13T10:01:01Z","abstract_excerpt":"The nature of solar wind turbulence in the dissipation range at scales much smaller than the large MHD scales remains under debate. Here a two-dimensional model based on the hybrid code abbreviated as A.I.K.E.F. is presented, which treats massive ions as particles obeying the kinetic Vlasov equation and massless electrons as a neutralizing fluid. Up to a certain wavenumber in the MHD regime, the numerical system is initialized by assuming a superposition of isotropic Alfv\\'en waves with amplitudes that follow the empirically confirmed spectral law of Kolmogorov. Then turbulence develops and en"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.2784","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":"1201.2784","created_at":"2026-05-18T04:02:03.623292+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.2784v2","created_at":"2026-05-18T04:02:03.623292+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.2784","created_at":"2026-05-18T04:02:03.623292+00:00"},{"alias_kind":"pith_short_12","alias_value":"YAACHAFCPGRQ","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_16","alias_value":"YAACHAFCPGRQTL3M","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_8","alias_value":"YAACHAFC","created_at":"2026-05-18T12:27:27.928770+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/YAACHAFCPGRQTL3MCISMYBSBBE","json":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE.json","graph_json":"https://pith.science/api/pith-number/YAACHAFCPGRQTL3MCISMYBSBBE/graph.json","events_json":"https://pith.science/api/pith-number/YAACHAFCPGRQTL3MCISMYBSBBE/events.json","paper":"https://pith.science/paper/YAACHAFC"},"agent_actions":{"view_html":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE","download_json":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE.json","view_paper":"https://pith.science/paper/YAACHAFC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.2784&json=true","fetch_graph":"https://pith.science/api/pith-number/YAACHAFCPGRQTL3MCISMYBSBBE/graph.json","fetch_events":"https://pith.science/api/pith-number/YAACHAFCPGRQTL3MCISMYBSBBE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE/action/storage_attestation","attest_author":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE/action/author_attestation","sign_citation":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE/action/citation_signature","submit_replication":"https://pith.science/pith/YAACHAFCPGRQTL3MCISMYBSBBE/action/replication_record"}},"created_at":"2026-05-18T04:02:03.623292+00:00","updated_at":"2026-05-18T04:02:03.623292+00:00"}