{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:DT4ZZTA4UPTYLCA4A75AGVHKZQ","short_pith_number":"pith:DT4ZZTA4","canonical_record":{"source":{"id":"1608.05161","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-08-18T03:11:02Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"823f77407d5c9f0a52aa7040c8eebbb848a2d8f1ed596f3c1819965743645487","abstract_canon_sha256":"eb8f9833c6d5170a3f43150606aa47197fc5b08071edbba8a357c0abbc607d5a"},"schema_version":"1.0"},"canonical_sha256":"1cf99ccc1ca3e785881c07fa0354eacc13e3c4a00eb8fc72c32a2449bdb4ed39","source":{"kind":"arxiv","id":"1608.05161","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1608.05161","created_at":"2026-05-18T00:53:59Z"},{"alias_kind":"arxiv_version","alias_value":"1608.05161v2","created_at":"2026-05-18T00:53:59Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.05161","created_at":"2026-05-18T00:53:59Z"},{"alias_kind":"pith_short_12","alias_value":"DT4ZZTA4UPTY","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_16","alias_value":"DT4ZZTA4UPTYLCA4","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_8","alias_value":"DT4ZZTA4","created_at":"2026-05-18T12:30:12Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:DT4ZZTA4UPTYLCA4A75AGVHKZQ","target":"record","payload":{"canonical_record":{"source":{"id":"1608.05161","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-08-18T03:11:02Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"823f77407d5c9f0a52aa7040c8eebbb848a2d8f1ed596f3c1819965743645487","abstract_canon_sha256":"eb8f9833c6d5170a3f43150606aa47197fc5b08071edbba8a357c0abbc607d5a"},"schema_version":"1.0"},"canonical_sha256":"1cf99ccc1ca3e785881c07fa0354eacc13e3c4a00eb8fc72c32a2449bdb4ed39","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:59.277927Z","signature_b64":"oSTSdApiKIi6eXd1WDMh1XLN/ANRmxbCENgfQW9GEOjAE4v0jCgyd35mV73G0kHNB70dcA3qsNAPzE7iizsCCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1cf99ccc1ca3e785881c07fa0354eacc13e3c4a00eb8fc72c32a2449bdb4ed39","last_reissued_at":"2026-05-18T00:53:59.277164Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:59.277164Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1608.05161","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:53:59Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"g+6zMzdi7cNGuz0qJP1InjGxR2+w8+8C3t5IB5oWNG/BeCbder8mOm3wQUlExvFvtLqD7jwHR3vcA9HB0h4aCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T18:29:22.831016Z"},"content_sha256":"74f03d31bbeb6d74261499c8884492125535c063064ff33316a5cde327df4eea","schema_version":"1.0","event_id":"sha256:74f03d31bbeb6d74261499c8884492125535c063064ff33316a5cde327df4eea"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:DT4ZZTA4UPTYLCA4A75AGVHKZQ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Turbulent dynamo in a conducting fluid and partially ionized gas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.GA","authors_text":"A. Lazarian, Siyao Xu","submitted_at":"2016-08-18T03:11:02Z","abstract_excerpt":"By following the Kazantsev theory and taking into account both microscopic and turbulent diffusion of magnetic fields, we develop a unified treatment of the kinematic and nonlinear stages of turbulent dynamo, and study the dynamo process for a full range of magnetic Prandtl number Pm and ionization fractions. We find a striking similarity between the dependence of dynamo behavior on Pm in a conducting fluid and R (a function of ionization fraction) in partially ionized gas. In a weakly ionized medium, the kinematic stage is largely extended, including not only exponential growth but a new regi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.05161","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:53:59Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"rd+/srBKE54noPBOPJKRcpWfu/XHnnqAVaqFa7wdFmbMiDFLGxDoaieFkAvhu6dQV1O07hRU+8vZbptzhd3eAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T18:29:22.831701Z"},"content_sha256":"204592febecf8ec6e17a34c4f77d4645cf0d7969944ea5835b08459513f9b6ce","schema_version":"1.0","event_id":"sha256:204592febecf8ec6e17a34c4f77d4645cf0d7969944ea5835b08459513f9b6ce"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/DT4ZZTA4UPTYLCA4A75AGVHKZQ/bundle.json","state_url":"https://pith.science/pith/DT4ZZTA4UPTYLCA4A75AGVHKZQ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/DT4ZZTA4UPTYLCA4A75AGVHKZQ/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":"2026-05-28T18:29:22Z","links":{"resolver":"https://pith.science/pith/DT4ZZTA4UPTYLCA4A75AGVHKZQ","bundle":"https://pith.science/pith/DT4ZZTA4UPTYLCA4A75AGVHKZQ/bundle.json","state":"https://pith.science/pith/DT4ZZTA4UPTYLCA4A75AGVHKZQ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/DT4ZZTA4UPTYLCA4A75AGVHKZQ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:DT4ZZTA4UPTYLCA4A75AGVHKZQ","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":"eb8f9833c6d5170a3f43150606aa47197fc5b08071edbba8a357c0abbc607d5a","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-08-18T03:11:02Z","title_canon_sha256":"823f77407d5c9f0a52aa7040c8eebbb848a2d8f1ed596f3c1819965743645487"},"schema_version":"1.0","source":{"id":"1608.05161","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1608.05161","created_at":"2026-05-18T00:53:59Z"},{"alias_kind":"arxiv_version","alias_value":"1608.05161v2","created_at":"2026-05-18T00:53:59Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.05161","created_at":"2026-05-18T00:53:59Z"},{"alias_kind":"pith_short_12","alias_value":"DT4ZZTA4UPTY","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_16","alias_value":"DT4ZZTA4UPTYLCA4","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_8","alias_value":"DT4ZZTA4","created_at":"2026-05-18T12:30:12Z"}],"graph_snapshots":[{"event_id":"sha256:204592febecf8ec6e17a34c4f77d4645cf0d7969944ea5835b08459513f9b6ce","target":"graph","created_at":"2026-05-18T00:53:59Z","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":"By following the Kazantsev theory and taking into account both microscopic and turbulent diffusion of magnetic fields, we develop a unified treatment of the kinematic and nonlinear stages of turbulent dynamo, and study the dynamo process for a full range of magnetic Prandtl number Pm and ionization fractions. We find a striking similarity between the dependence of dynamo behavior on Pm in a conducting fluid and R (a function of ionization fraction) in partially ionized gas. In a weakly ionized medium, the kinematic stage is largely extended, including not only exponential growth but a new regi","authors_text":"A. Lazarian, Siyao Xu","cross_cats":["physics.plasm-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-08-18T03:11:02Z","title":"Turbulent dynamo in a conducting fluid and partially ionized gas"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.05161","kind":"arxiv","version":2},"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":"sha256:74f03d31bbeb6d74261499c8884492125535c063064ff33316a5cde327df4eea","target":"record","created_at":"2026-05-18T00:53:59Z","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":"eb8f9833c6d5170a3f43150606aa47197fc5b08071edbba8a357c0abbc607d5a","cross_cats_sorted":["physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-08-18T03:11:02Z","title_canon_sha256":"823f77407d5c9f0a52aa7040c8eebbb848a2d8f1ed596f3c1819965743645487"},"schema_version":"1.0","source":{"id":"1608.05161","kind":"arxiv","version":2}},"canonical_sha256":"1cf99ccc1ca3e785881c07fa0354eacc13e3c4a00eb8fc72c32a2449bdb4ed39","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"1cf99ccc1ca3e785881c07fa0354eacc13e3c4a00eb8fc72c32a2449bdb4ed39","first_computed_at":"2026-05-18T00:53:59.277164Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:53:59.277164Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"oSTSdApiKIi6eXd1WDMh1XLN/ANRmxbCENgfQW9GEOjAE4v0jCgyd35mV73G0kHNB70dcA3qsNAPzE7iizsCCw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:53:59.277927Z","signed_message":"canonical_sha256_bytes"},"source_id":"1608.05161","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:74f03d31bbeb6d74261499c8884492125535c063064ff33316a5cde327df4eea","sha256:204592febecf8ec6e17a34c4f77d4645cf0d7969944ea5835b08459513f9b6ce"],"state_sha256":"4a1a164a4d4afa00ba35941201e2ee2e36b8ca71f67a4baac865ebb104fc0320"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Di0H095UVUyckuKpvO9eqbMzoMZ5guOJXj8G2y6ZpCl09a6oXRIz4ridk5LNQFRUAEG5pH8HeYdMv6mtcNMLAQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T18:29:22.835417Z","bundle_sha256":"0016bd28f598f4df9e9a401413c4d7a9d743aab7df4fc1b327a3508983391e5d"}}