{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:BRNCTBAH6A756MHKGMAMY4JVT2","short_pith_number":"pith:BRNCTBAH","canonical_record":{"source":{"id":"1109.4158","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-09-19T20:08:53Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"4f79145c4acab65b86b730791a4e8198d35586849324370e9305afdb2156bd73","abstract_canon_sha256":"76488a1a9cb3e44f9244d7a9ee4b93399741184ff9d3ff62e370dbb7edae906a"},"schema_version":"1.0"},"canonical_sha256":"0c5a298407f03fdf30ea3300cc71359e8bff4b00e64ea039f7cfa7e5481d6e7a","source":{"kind":"arxiv","id":"1109.4158","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1109.4158","created_at":"2026-05-18T02:00:29Z"},{"alias_kind":"arxiv_version","alias_value":"1109.4158v1","created_at":"2026-05-18T02:00:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.4158","created_at":"2026-05-18T02:00:29Z"},{"alias_kind":"pith_short_12","alias_value":"BRNCTBAH6A75","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_16","alias_value":"BRNCTBAH6A756MHK","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_8","alias_value":"BRNCTBAH","created_at":"2026-05-18T12:26:24Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:BRNCTBAH6A756MHKGMAMY4JVT2","target":"record","payload":{"canonical_record":{"source":{"id":"1109.4158","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-09-19T20:08:53Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"4f79145c4acab65b86b730791a4e8198d35586849324370e9305afdb2156bd73","abstract_canon_sha256":"76488a1a9cb3e44f9244d7a9ee4b93399741184ff9d3ff62e370dbb7edae906a"},"schema_version":"1.0"},"canonical_sha256":"0c5a298407f03fdf30ea3300cc71359e8bff4b00e64ea039f7cfa7e5481d6e7a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:29.057232Z","signature_b64":"2VkRAGP07Yd9hiwWYTcr7gr6wKUTYsPxekiAM6kZJGfIcfzIFuSVTDv3DwVdFncwv9ubxtlXtUAEN7D3XUFRAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c5a298407f03fdf30ea3300cc71359e8bff4b00e64ea039f7cfa7e5481d6e7a","last_reissued_at":"2026-05-18T02:00:29.056663Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:29.056663Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1109.4158","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:00:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"nehJosbWcc37iKqKhnqHXIekRRazRPaFeZk0tv+fFLF0hhSntNUSq7hpx5Z9IBc0e99zRJbKHdZjm0KAon3+Cw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T19:42:29.203153Z"},"content_sha256":"acc5f9fec535c1bb3c9167a7a7e3bcef278439a0813503606310ce024b8350ef","schema_version":"1.0","event_id":"sha256:acc5f9fec535c1bb3c9167a7a7e3bcef278439a0813503606310ce024b8350ef"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:BRNCTBAH6A756MHKGMAMY4JVT2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A Weakened Cascade Model for Turbulence in Astrophysical Plasmas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.SR","authors_text":"G. G. Howes, J. M. TenBarge, W. Dorland","submitted_at":"2011-09-19T20:08:53Z","abstract_excerpt":"A refined cascade model for kinetic turbulence in weakly collisional astrophysical plasmas is presented that includes both the transition between weak and strong turbulence and the effect of nonlocal interactions on the nonlinear transfer of energy. The model describes the transition between weak and strong MHD turbulence and the complementary transition from strong kinetic Alfven wave (KAW) turbulence to weak dissipating KAW turbulence, a new regime of weak turbulence in which the effects of shearing by large scale motions and kinetic dissipation play an important role. The inclusion of the e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.4158","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:00:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"YWiS5jLQFpGAQLxtxbpUXnca4Vj4q0PYBfi4Iw7FXoutWcAShNc7SR5+YEggCQtvgHPdFD838T+Rih1uLeS5BQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T19:42:29.203780Z"},"content_sha256":"bd80a07e04b1607c5966ec0f1cad398c71e7d441ab6681c4e34828411e0df9f8","schema_version":"1.0","event_id":"sha256:bd80a07e04b1607c5966ec0f1cad398c71e7d441ab6681c4e34828411e0df9f8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/BRNCTBAH6A756MHKGMAMY4JVT2/bundle.json","state_url":"https://pith.science/pith/BRNCTBAH6A756MHKGMAMY4JVT2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/BRNCTBAH6A756MHKGMAMY4JVT2/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-27T19:42:29Z","links":{"resolver":"https://pith.science/pith/BRNCTBAH6A756MHKGMAMY4JVT2","bundle":"https://pith.science/pith/BRNCTBAH6A756MHKGMAMY4JVT2/bundle.json","state":"https://pith.science/pith/BRNCTBAH6A756MHKGMAMY4JVT2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/BRNCTBAH6A756MHKGMAMY4JVT2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:BRNCTBAH6A756MHKGMAMY4JVT2","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"76488a1a9cb3e44f9244d7a9ee4b93399741184ff9d3ff62e370dbb7edae906a","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-09-19T20:08:53Z","title_canon_sha256":"4f79145c4acab65b86b730791a4e8198d35586849324370e9305afdb2156bd73"},"schema_version":"1.0","source":{"id":"1109.4158","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1109.4158","created_at":"2026-05-18T02:00:29Z"},{"alias_kind":"arxiv_version","alias_value":"1109.4158v1","created_at":"2026-05-18T02:00:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.4158","created_at":"2026-05-18T02:00:29Z"},{"alias_kind":"pith_short_12","alias_value":"BRNCTBAH6A75","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_16","alias_value":"BRNCTBAH6A756MHK","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_8","alias_value":"BRNCTBAH","created_at":"2026-05-18T12:26:24Z"}],"graph_snapshots":[{"event_id":"sha256:bd80a07e04b1607c5966ec0f1cad398c71e7d441ab6681c4e34828411e0df9f8","target":"graph","created_at":"2026-05-18T02:00:29Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"A refined cascade model for kinetic turbulence in weakly collisional astrophysical plasmas is presented that includes both the transition between weak and strong turbulence and the effect of nonlocal interactions on the nonlinear transfer of energy. The model describes the transition between weak and strong MHD turbulence and the complementary transition from strong kinetic Alfven wave (KAW) turbulence to weak dissipating KAW turbulence, a new regime of weak turbulence in which the effects of shearing by large scale motions and kinetic dissipation play an important role. The inclusion of the e","authors_text":"G. G. Howes, J. M. TenBarge, W. Dorland","cross_cats":["physics.plasm-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-09-19T20:08:53Z","title":"A Weakened Cascade Model for Turbulence in Astrophysical Plasmas"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.4158","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:acc5f9fec535c1bb3c9167a7a7e3bcef278439a0813503606310ce024b8350ef","target":"record","created_at":"2026-05-18T02:00:29Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"76488a1a9cb3e44f9244d7a9ee4b93399741184ff9d3ff62e370dbb7edae906a","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-09-19T20:08:53Z","title_canon_sha256":"4f79145c4acab65b86b730791a4e8198d35586849324370e9305afdb2156bd73"},"schema_version":"1.0","source":{"id":"1109.4158","kind":"arxiv","version":1}},"canonical_sha256":"0c5a298407f03fdf30ea3300cc71359e8bff4b00e64ea039f7cfa7e5481d6e7a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"0c5a298407f03fdf30ea3300cc71359e8bff4b00e64ea039f7cfa7e5481d6e7a","first_computed_at":"2026-05-18T02:00:29.056663Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:00:29.056663Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"2VkRAGP07Yd9hiwWYTcr7gr6wKUTYsPxekiAM6kZJGfIcfzIFuSVTDv3DwVdFncwv9ubxtlXtUAEN7D3XUFRAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:00:29.057232Z","signed_message":"canonical_sha256_bytes"},"source_id":"1109.4158","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:acc5f9fec535c1bb3c9167a7a7e3bcef278439a0813503606310ce024b8350ef","sha256:bd80a07e04b1607c5966ec0f1cad398c71e7d441ab6681c4e34828411e0df9f8"],"state_sha256":"007132ff74e51db8f65450a1d153630b67984936ee6772f763cb5258a9a6d6c8"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"FFhNdM4o5OwXCt0akygPHYo0qFuvBOQueutMznPtG0sTa6BkzqQEDzaNk6INXbTUIXjR/UVe+V8NBQK9PcQpCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T19:42:29.206259Z","bundle_sha256":"a6619925efa9ba25ef3f7aac00d2333009f18b6bebf0031b0c7ea7a840d852b0"}}