{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:JUPYIWU24LUOKJZYPONPCB2OPK","short_pith_number":"pith:JUPYIWU2","canonical_record":{"source":{"id":"1812.02379","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-12-06T07:13:58Z","cross_cats_sorted":["physics.flu-dyn","physics.space-ph"],"title_canon_sha256":"19080dc7fe6b4a7ee596e18b8db5f241458f0c4c53fa6977f8cb300947bf41cf","abstract_canon_sha256":"05f4e10ad079b9405ca851c27ffb08ae489350802d45603805897aa5a69d605b"},"schema_version":"1.0"},"canonical_sha256":"4d1f845a9ae2e8e527387b9af1074e7aa830947ff09c2bc554bb67ea51c0e308","source":{"kind":"arxiv","id":"1812.02379","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1812.02379","created_at":"2026-05-17T23:58:56Z"},{"alias_kind":"arxiv_version","alias_value":"1812.02379v1","created_at":"2026-05-17T23:58:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.02379","created_at":"2026-05-17T23:58:56Z"},{"alias_kind":"pith_short_12","alias_value":"JUPYIWU24LUO","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JUPYIWU24LUOKJZY","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JUPYIWU2","created_at":"2026-05-18T12:32:31Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:JUPYIWU24LUOKJZYPONPCB2OPK","target":"record","payload":{"canonical_record":{"source":{"id":"1812.02379","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-12-06T07:13:58Z","cross_cats_sorted":["physics.flu-dyn","physics.space-ph"],"title_canon_sha256":"19080dc7fe6b4a7ee596e18b8db5f241458f0c4c53fa6977f8cb300947bf41cf","abstract_canon_sha256":"05f4e10ad079b9405ca851c27ffb08ae489350802d45603805897aa5a69d605b"},"schema_version":"1.0"},"canonical_sha256":"4d1f845a9ae2e8e527387b9af1074e7aa830947ff09c2bc554bb67ea51c0e308","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:56.461576Z","signature_b64":"7Pq86R2DJ7tUG9d3x5/dDaociA7ihxq8hju0jTZVf8+rQDJMa/+uCTRcZZ3/AATdObz2FJIOLqXI7tg8doIMAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4d1f845a9ae2e8e527387b9af1074e7aa830947ff09c2bc554bb67ea51c0e308","last_reissued_at":"2026-05-17T23:58:56.461011Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:56.461011Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1812.02379","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":"2026-05-17T23:58:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uEIf1QPoXReEh3Qsp06Av7dRJkvGum9yIuOEIICRJuMsCuaIYC6xf7mPG99OakoNvkBTtcaWb/JYKX9T5YW9Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T14:42:52.699950Z"},"content_sha256":"754351199337e40a3681bd4a27bdcc86896e8555aced21badeff01c30d8ac20f","schema_version":"1.0","event_id":"sha256:754351199337e40a3681bd4a27bdcc86896e8555aced21badeff01c30d8ac20f"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:JUPYIWU24LUOKJZYPONPCB2OPK","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Finite Dissipation in Anisotropic Magnetohydrodynamic Turbulence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.flu-dyn","physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"M. Wan, R. Chhiber, Riddhi Bandyopadhyay, S. Oughton, T. N. Parashar, W. H. Matthaeus","submitted_at":"2018-12-06T07:13:58Z","abstract_excerpt":"In presence of an externally supported, mean magnetic field a turbulent, conducting medium, such as plasma, becomes anisotropic. This mean magnetic field, which is separate from the fluctuating, turbulent part of the magnetic field, has considerable effects on the dynamics of the system. In this paper, we examine the dissipation rates for decaying incompressible magnetohydrodynamic (MHD) turbulence with increasing Reynolds number, and in the presence of a mean magnetic field of varying strength. Proceeding numerically, we find that as the Reynolds number increases, the dissipation rate asympto"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.02379","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":"2026-05-17T23:58:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1vHK7vK1rzNe+5HTzunIebWlm7ZFaBj2LGxa0GUAD2dIEQnFGeHEfw96R/IBxErrLCTzsXeupd4FMXspG3aDCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T14:42:52.700660Z"},"content_sha256":"0374b35730e462de2cd50d74e93a5e82ef7db4615ae270d22c3ba17458285389","schema_version":"1.0","event_id":"sha256:0374b35730e462de2cd50d74e93a5e82ef7db4615ae270d22c3ba17458285389"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/JUPYIWU24LUOKJZYPONPCB2OPK/bundle.json","state_url":"https://pith.science/pith/JUPYIWU24LUOKJZYPONPCB2OPK/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/JUPYIWU24LUOKJZYPONPCB2OPK/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":"2026-05-25T14:42:52Z","links":{"resolver":"https://pith.science/pith/JUPYIWU24LUOKJZYPONPCB2OPK","bundle":"https://pith.science/pith/JUPYIWU24LUOKJZYPONPCB2OPK/bundle.json","state":"https://pith.science/pith/JUPYIWU24LUOKJZYPONPCB2OPK/state.json","well_known_bundle":"https://pith.science/.well-known/pith/JUPYIWU24LUOKJZYPONPCB2OPK/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:JUPYIWU24LUOKJZYPONPCB2OPK","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":"05f4e10ad079b9405ca851c27ffb08ae489350802d45603805897aa5a69d605b","cross_cats_sorted":["physics.flu-dyn","physics.space-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-12-06T07:13:58Z","title_canon_sha256":"19080dc7fe6b4a7ee596e18b8db5f241458f0c4c53fa6977f8cb300947bf41cf"},"schema_version":"1.0","source":{"id":"1812.02379","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1812.02379","created_at":"2026-05-17T23:58:56Z"},{"alias_kind":"arxiv_version","alias_value":"1812.02379v1","created_at":"2026-05-17T23:58:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.02379","created_at":"2026-05-17T23:58:56Z"},{"alias_kind":"pith_short_12","alias_value":"JUPYIWU24LUO","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JUPYIWU24LUOKJZY","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JUPYIWU2","created_at":"2026-05-18T12:32:31Z"}],"graph_snapshots":[{"event_id":"sha256:0374b35730e462de2cd50d74e93a5e82ef7db4615ae270d22c3ba17458285389","target":"graph","created_at":"2026-05-17T23:58:56Z","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":"In presence of an externally supported, mean magnetic field a turbulent, conducting medium, such as plasma, becomes anisotropic. This mean magnetic field, which is separate from the fluctuating, turbulent part of the magnetic field, has considerable effects on the dynamics of the system. In this paper, we examine the dissipation rates for decaying incompressible magnetohydrodynamic (MHD) turbulence with increasing Reynolds number, and in the presence of a mean magnetic field of varying strength. Proceeding numerically, we find that as the Reynolds number increases, the dissipation rate asympto","authors_text":"M. Wan, R. Chhiber, Riddhi Bandyopadhyay, S. Oughton, T. N. Parashar, W. H. Matthaeus","cross_cats":["physics.flu-dyn","physics.space-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-12-06T07:13:58Z","title":"Finite Dissipation in Anisotropic Magnetohydrodynamic Turbulence"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.02379","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":"sha256:754351199337e40a3681bd4a27bdcc86896e8555aced21badeff01c30d8ac20f","target":"record","created_at":"2026-05-17T23:58:56Z","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":"05f4e10ad079b9405ca851c27ffb08ae489350802d45603805897aa5a69d605b","cross_cats_sorted":["physics.flu-dyn","physics.space-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-12-06T07:13:58Z","title_canon_sha256":"19080dc7fe6b4a7ee596e18b8db5f241458f0c4c53fa6977f8cb300947bf41cf"},"schema_version":"1.0","source":{"id":"1812.02379","kind":"arxiv","version":1}},"canonical_sha256":"4d1f845a9ae2e8e527387b9af1074e7aa830947ff09c2bc554bb67ea51c0e308","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"4d1f845a9ae2e8e527387b9af1074e7aa830947ff09c2bc554bb67ea51c0e308","first_computed_at":"2026-05-17T23:58:56.461011Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:58:56.461011Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"7Pq86R2DJ7tUG9d3x5/dDaociA7ihxq8hju0jTZVf8+rQDJMa/+uCTRcZZ3/AATdObz2FJIOLqXI7tg8doIMAw==","signature_status":"signed_v1","signed_at":"2026-05-17T23:58:56.461576Z","signed_message":"canonical_sha256_bytes"},"source_id":"1812.02379","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:754351199337e40a3681bd4a27bdcc86896e8555aced21badeff01c30d8ac20f","sha256:0374b35730e462de2cd50d74e93a5e82ef7db4615ae270d22c3ba17458285389"],"state_sha256":"fbcb347bb91741f0a768fac0982ea6d3315981398d011d734bf2340d5fe32211"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"vCJKNMtEfFOm26oeXwrcqavcuwDmxXp+kbDjCDwI6qOTbwnI2ETXleZMBdKTCLyPWjXayCPBrS05knGCsoTzCw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T14:42:52.704157Z","bundle_sha256":"0d9abbd78dbaae110b9589e1fe784edb68c338e1e8a3b5f8a04cd6e0d575aa14"}}