{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2019:HO6RNNKFEHLMGNN2SZTSZDQSOF","short_pith_number":"pith:HO6RNNKF","canonical_record":{"source":{"id":"1906.04821","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-06-11T21:01:22Z","cross_cats_sorted":[],"title_canon_sha256":"8e2f05e0c9856b901bcccb891547891732e909998c02075a37c47554ffd144a5","abstract_canon_sha256":"b28bdb67f1bb93b816c77bbe832298445f1c16658b03b11d17114aa33c45ec82"},"schema_version":"1.0"},"canonical_sha256":"3bbd16b54521d6c335ba96672c8e12716749a17e7ce2fcf5b58035fad21e2b08","source":{"kind":"arxiv","id":"1906.04821","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1906.04821","created_at":"2026-05-17T23:43:30Z"},{"alias_kind":"arxiv_version","alias_value":"1906.04821v1","created_at":"2026-05-17T23:43:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.04821","created_at":"2026-05-17T23:43:30Z"},{"alias_kind":"pith_short_12","alias_value":"HO6RNNKFEHLM","created_at":"2026-05-18T12:33:18Z"},{"alias_kind":"pith_short_16","alias_value":"HO6RNNKFEHLMGNN2","created_at":"2026-05-18T12:33:18Z"},{"alias_kind":"pith_short_8","alias_value":"HO6RNNKF","created_at":"2026-05-18T12:33:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2019:HO6RNNKFEHLMGNN2SZTSZDQSOF","target":"record","payload":{"canonical_record":{"source":{"id":"1906.04821","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-06-11T21:01:22Z","cross_cats_sorted":[],"title_canon_sha256":"8e2f05e0c9856b901bcccb891547891732e909998c02075a37c47554ffd144a5","abstract_canon_sha256":"b28bdb67f1bb93b816c77bbe832298445f1c16658b03b11d17114aa33c45ec82"},"schema_version":"1.0"},"canonical_sha256":"3bbd16b54521d6c335ba96672c8e12716749a17e7ce2fcf5b58035fad21e2b08","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:43:30.410433Z","signature_b64":"YovRiFbzW9Z6YfKotSTMgq3C0Womx7BY0vNrwEsKipyy3RQpWWqkbRyNztrXMBOWzTzryYTp851kvOlP4548DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3bbd16b54521d6c335ba96672c8e12716749a17e7ce2fcf5b58035fad21e2b08","last_reissued_at":"2026-05-17T23:43:30.410048Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:43:30.410048Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1906.04821","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":"2026-05-17T23:43:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"BsIp8R8HIcJ/ii4/vbaVgerc1oXqR3lAHXyHsMdNvLB0uxTAUulzWy8T9+DmSm97ZmQ6lmoRlZ5QnqAkJ0mdDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-06T10:42:54.496105Z"},"content_sha256":"da3a3051c1b1bc83c6a79d54ec1ee2e779965364650a703c87c0a286adf1577c","schema_version":"1.0","event_id":"sha256:da3a3051c1b1bc83c6a79d54ec1ee2e779965364650a703c87c0a286adf1577c"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2019:HO6RNNKFEHLMGNN2SZTSZDQSOF","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Effects of the magnetic field direction on the Tsallis statistic","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Lazarian, Diego F. Gonz\\'alez-Casanova, J. Cho","submitted_at":"2019-06-11T21:01:22Z","abstract_excerpt":"We extend the use of the Tsallis statistic to measure the differences in gas dynamics relative to the mean magnetic field present from natural eddy-type motions existing in magnetohydrodynamical (MHD) turbulence. The variation in gas dynamics was estimated using the Tsallis parameters on the incremental probability distribution function of the observables (intensity and velocity centroid) obtained from compressible MHD simulations. We find that the Tsallis statistic is susceptible to the anisotropy produce by the magnetic field, even when anisotropy is percent the Tsallis statistic can be use "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.04821","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":"2026-05-17T23:43:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AGix2OGOgF9+uMaVbBEGWOzZI81ax3ZJCgfSVQmT6Th7LQmR0VeFC3V27zh2NW6Bv/Y3ZhvQNPFHoVV5HqyMBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-06T10:42:54.496469Z"},"content_sha256":"234e4fe1526543bce67bf3c7a8c3a3ad7c4d1b598e3a3c2a3b9409a0c5864b5e","schema_version":"1.0","event_id":"sha256:234e4fe1526543bce67bf3c7a8c3a3ad7c4d1b598e3a3c2a3b9409a0c5864b5e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/HO6RNNKFEHLMGNN2SZTSZDQSOF/bundle.json","state_url":"https://pith.science/pith/HO6RNNKFEHLMGNN2SZTSZDQSOF/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/HO6RNNKFEHLMGNN2SZTSZDQSOF/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":"2026-07-06T10:42:54Z","links":{"resolver":"https://pith.science/pith/HO6RNNKFEHLMGNN2SZTSZDQSOF","bundle":"https://pith.science/pith/HO6RNNKFEHLMGNN2SZTSZDQSOF/bundle.json","state":"https://pith.science/pith/HO6RNNKFEHLMGNN2SZTSZDQSOF/state.json","well_known_bundle":"https://pith.science/.well-known/pith/HO6RNNKFEHLMGNN2SZTSZDQSOF/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2019:HO6RNNKFEHLMGNN2SZTSZDQSOF","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":"b28bdb67f1bb93b816c77bbe832298445f1c16658b03b11d17114aa33c45ec82","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-06-11T21:01:22Z","title_canon_sha256":"8e2f05e0c9856b901bcccb891547891732e909998c02075a37c47554ffd144a5"},"schema_version":"1.0","source":{"id":"1906.04821","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1906.04821","created_at":"2026-05-17T23:43:30Z"},{"alias_kind":"arxiv_version","alias_value":"1906.04821v1","created_at":"2026-05-17T23:43:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.04821","created_at":"2026-05-17T23:43:30Z"},{"alias_kind":"pith_short_12","alias_value":"HO6RNNKFEHLM","created_at":"2026-05-18T12:33:18Z"},{"alias_kind":"pith_short_16","alias_value":"HO6RNNKFEHLMGNN2","created_at":"2026-05-18T12:33:18Z"},{"alias_kind":"pith_short_8","alias_value":"HO6RNNKF","created_at":"2026-05-18T12:33:18Z"}],"graph_snapshots":[{"event_id":"sha256:234e4fe1526543bce67bf3c7a8c3a3ad7c4d1b598e3a3c2a3b9409a0c5864b5e","target":"graph","created_at":"2026-05-17T23:43:30Z","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":"We extend the use of the Tsallis statistic to measure the differences in gas dynamics relative to the mean magnetic field present from natural eddy-type motions existing in magnetohydrodynamical (MHD) turbulence. The variation in gas dynamics was estimated using the Tsallis parameters on the incremental probability distribution function of the observables (intensity and velocity centroid) obtained from compressible MHD simulations. We find that the Tsallis statistic is susceptible to the anisotropy produce by the magnetic field, even when anisotropy is percent the Tsallis statistic can be use ","authors_text":"A. Lazarian, Diego F. Gonz\\'alez-Casanova, J. Cho","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-06-11T21:01:22Z","title":"Effects of the magnetic field direction on the Tsallis statistic"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.04821","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:da3a3051c1b1bc83c6a79d54ec1ee2e779965364650a703c87c0a286adf1577c","target":"record","created_at":"2026-05-17T23:43:30Z","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":"b28bdb67f1bb93b816c77bbe832298445f1c16658b03b11d17114aa33c45ec82","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-06-11T21:01:22Z","title_canon_sha256":"8e2f05e0c9856b901bcccb891547891732e909998c02075a37c47554ffd144a5"},"schema_version":"1.0","source":{"id":"1906.04821","kind":"arxiv","version":1}},"canonical_sha256":"3bbd16b54521d6c335ba96672c8e12716749a17e7ce2fcf5b58035fad21e2b08","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3bbd16b54521d6c335ba96672c8e12716749a17e7ce2fcf5b58035fad21e2b08","first_computed_at":"2026-05-17T23:43:30.410048Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:43:30.410048Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"YovRiFbzW9Z6YfKotSTMgq3C0Womx7BY0vNrwEsKipyy3RQpWWqkbRyNztrXMBOWzTzryYTp851kvOlP4548DQ==","signature_status":"signed_v1","signed_at":"2026-05-17T23:43:30.410433Z","signed_message":"canonical_sha256_bytes"},"source_id":"1906.04821","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:da3a3051c1b1bc83c6a79d54ec1ee2e779965364650a703c87c0a286adf1577c","sha256:234e4fe1526543bce67bf3c7a8c3a3ad7c4d1b598e3a3c2a3b9409a0c5864b5e"],"state_sha256":"d8ad410e724a42c8061881654e14fbdd68b34830ca58893147154ca6bb582393"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"/5+oZzJ7ynJcYjrNxbLeT3+F+p8vJwIdmC8AfZUqtExLdfA4TN7ttSlHKJFjYuUenuLfbb0eB+79fRHLsWrEBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-06T10:42:54.498493Z","bundle_sha256":"56554bba9033dac45618b800820866bfc2afc06a4d680fbde9eddfe9dc12c7b4"}}