{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:47NBJM7Z2NDVUQPEPFFEYZF7X2","short_pith_number":"pith:47NBJM7Z","canonical_record":{"source":{"id":"1508.01187","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2015-08-05T19:28:17Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"37ca89ba689bee3fbea4359b08639ecc0820eb7ab1ebbbac1754e3b6b036cfe0","abstract_canon_sha256":"9db67bffc3f5a3475672a4cfcfa9180c7c6ce99236e967b75eda6f025397105c"},"schema_version":"1.0"},"canonical_sha256":"e7da14b3f9d3475a41e4794a4c64bfbe8ca47d635719f22fab08bf433c86b62c","source":{"kind":"arxiv","id":"1508.01187","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1508.01187","created_at":"2026-05-18T01:27:22Z"},{"alias_kind":"arxiv_version","alias_value":"1508.01187v1","created_at":"2026-05-18T01:27:22Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.01187","created_at":"2026-05-18T01:27:22Z"},{"alias_kind":"pith_short_12","alias_value":"47NBJM7Z2NDV","created_at":"2026-05-18T12:29:05Z"},{"alias_kind":"pith_short_16","alias_value":"47NBJM7Z2NDVUQPE","created_at":"2026-05-18T12:29:05Z"},{"alias_kind":"pith_short_8","alias_value":"47NBJM7Z","created_at":"2026-05-18T12:29:05Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:47NBJM7Z2NDVUQPEPFFEYZF7X2","target":"record","payload":{"canonical_record":{"source":{"id":"1508.01187","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2015-08-05T19:28:17Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"37ca89ba689bee3fbea4359b08639ecc0820eb7ab1ebbbac1754e3b6b036cfe0","abstract_canon_sha256":"9db67bffc3f5a3475672a4cfcfa9180c7c6ce99236e967b75eda6f025397105c"},"schema_version":"1.0"},"canonical_sha256":"e7da14b3f9d3475a41e4794a4c64bfbe8ca47d635719f22fab08bf433c86b62c","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:27:22.931603Z","signature_b64":"7tpFNGiAtdxveEygh2wLcgP9YP4L18xk0Yq6/go16FEZ1FlGgfPuzs34+sFC6Ewc00B5RTBQI5TJis0hRraqDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7da14b3f9d3475a41e4794a4c64bfbe8ca47d635719f22fab08bf433c86b62c","last_reissued_at":"2026-05-18T01:27:22.931037Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:27:22.931037Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1508.01187","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":"2026-05-18T01:27:22Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8QXJRERCJ1jcaWC2salhcPPY/t5kNqH5AgXFfpv0AqwNrbVNVOPsLjFEvGUcR+hrH16QaDvygEal3ExRuQZbCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-02T05:00:33.247083Z"},"content_sha256":"14b3a31129be2d0753bf5c580fb581488a5d41c0a618a5d20f0c1bf895cb628d","schema_version":"1.0","event_id":"sha256:14b3a31129be2d0753bf5c580fb581488a5d41c0a618a5d20f0c1bf895cb628d"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:47NBJM7Z2NDVUQPEPFFEYZF7X2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"(Quasi-)collisional Magneto-optic Effects in Collisionless Plasmas with sub-Larmor-scale Electromagnetic Fluctuations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"physics.plasm-ph","authors_text":"Alexander L. Ford, Brett D. Keenan, Mikhail V. Medvedev","submitted_at":"2015-08-05T19:28:17Z","abstract_excerpt":"High-amplitude, chaotic/turbulent electromagnetic fluctuations are ubiquitous in high-energy-density laboratory and astrophysical plasmas, where they can be excited by various kinetic-streaming and/or anisotropy-driven instabilities, such as the Weibel instability. These fields typically exist on \"sub-Larmor scales\" -- scales smaller than the electron Larmor radius. Electrons moving through such magnetic fields undergo small-angle stochastic deflections of their pitch-angles, thus establishing diffusive transport on long time-scales. We show that this behavior, under certain conditions, is equ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.01187","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":"2026-05-18T01:27:22Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"KEmLUBvJnAqgwdgKrtIC6Vu6ONHAOtDnmvgAubMZhjrUn1jbXsPSpIyUg3Y8U9SXRPEZJAI0hhApsU7ET+OnAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-02T05:00:33.247444Z"},"content_sha256":"8fade0aa7de6f3892f6bf7e6b9661cbb5d76cb5d8fb5095fd3d44ae4e4489e79","schema_version":"1.0","event_id":"sha256:8fade0aa7de6f3892f6bf7e6b9661cbb5d76cb5d8fb5095fd3d44ae4e4489e79"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/47NBJM7Z2NDVUQPEPFFEYZF7X2/bundle.json","state_url":"https://pith.science/pith/47NBJM7Z2NDVUQPEPFFEYZF7X2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/47NBJM7Z2NDVUQPEPFFEYZF7X2/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":"2026-07-02T05:00:33Z","links":{"resolver":"https://pith.science/pith/47NBJM7Z2NDVUQPEPFFEYZF7X2","bundle":"https://pith.science/pith/47NBJM7Z2NDVUQPEPFFEYZF7X2/bundle.json","state":"https://pith.science/pith/47NBJM7Z2NDVUQPEPFFEYZF7X2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/47NBJM7Z2NDVUQPEPFFEYZF7X2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:47NBJM7Z2NDVUQPEPFFEYZF7X2","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":"9db67bffc3f5a3475672a4cfcfa9180c7c6ce99236e967b75eda6f025397105c","cross_cats_sorted":["astro-ph.IM"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2015-08-05T19:28:17Z","title_canon_sha256":"37ca89ba689bee3fbea4359b08639ecc0820eb7ab1ebbbac1754e3b6b036cfe0"},"schema_version":"1.0","source":{"id":"1508.01187","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1508.01187","created_at":"2026-05-18T01:27:22Z"},{"alias_kind":"arxiv_version","alias_value":"1508.01187v1","created_at":"2026-05-18T01:27:22Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.01187","created_at":"2026-05-18T01:27:22Z"},{"alias_kind":"pith_short_12","alias_value":"47NBJM7Z2NDV","created_at":"2026-05-18T12:29:05Z"},{"alias_kind":"pith_short_16","alias_value":"47NBJM7Z2NDVUQPE","created_at":"2026-05-18T12:29:05Z"},{"alias_kind":"pith_short_8","alias_value":"47NBJM7Z","created_at":"2026-05-18T12:29:05Z"}],"graph_snapshots":[{"event_id":"sha256:8fade0aa7de6f3892f6bf7e6b9661cbb5d76cb5d8fb5095fd3d44ae4e4489e79","target":"graph","created_at":"2026-05-18T01:27:22Z","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":"High-amplitude, chaotic/turbulent electromagnetic fluctuations are ubiquitous in high-energy-density laboratory and astrophysical plasmas, where they can be excited by various kinetic-streaming and/or anisotropy-driven instabilities, such as the Weibel instability. These fields typically exist on \"sub-Larmor scales\" -- scales smaller than the electron Larmor radius. Electrons moving through such magnetic fields undergo small-angle stochastic deflections of their pitch-angles, thus establishing diffusive transport on long time-scales. We show that this behavior, under certain conditions, is equ","authors_text":"Alexander L. Ford, Brett D. Keenan, Mikhail V. Medvedev","cross_cats":["astro-ph.IM"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2015-08-05T19:28:17Z","title":"(Quasi-)collisional Magneto-optic Effects in Collisionless Plasmas with sub-Larmor-scale Electromagnetic Fluctuations"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.01187","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":"sha256:14b3a31129be2d0753bf5c580fb581488a5d41c0a618a5d20f0c1bf895cb628d","target":"record","created_at":"2026-05-18T01:27:22Z","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":"9db67bffc3f5a3475672a4cfcfa9180c7c6ce99236e967b75eda6f025397105c","cross_cats_sorted":["astro-ph.IM"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2015-08-05T19:28:17Z","title_canon_sha256":"37ca89ba689bee3fbea4359b08639ecc0820eb7ab1ebbbac1754e3b6b036cfe0"},"schema_version":"1.0","source":{"id":"1508.01187","kind":"arxiv","version":1}},"canonical_sha256":"e7da14b3f9d3475a41e4794a4c64bfbe8ca47d635719f22fab08bf433c86b62c","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"e7da14b3f9d3475a41e4794a4c64bfbe8ca47d635719f22fab08bf433c86b62c","first_computed_at":"2026-05-18T01:27:22.931037Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:27:22.931037Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"7tpFNGiAtdxveEygh2wLcgP9YP4L18xk0Yq6/go16FEZ1FlGgfPuzs34+sFC6Ewc00B5RTBQI5TJis0hRraqDQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:27:22.931603Z","signed_message":"canonical_sha256_bytes"},"source_id":"1508.01187","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:14b3a31129be2d0753bf5c580fb581488a5d41c0a618a5d20f0c1bf895cb628d","sha256:8fade0aa7de6f3892f6bf7e6b9661cbb5d76cb5d8fb5095fd3d44ae4e4489e79"],"state_sha256":"a07fc12340727f028a7ac168ef66522c51abe9c7d211361c058c4701e845015a"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"h/5u331pes8EKV1P1sl7gDpwJm70YvHw4O2u4kx7g6Bin+prjhOIntS+ZYvmgNTiy8LuVgUiYJB/mrDGQQ7ZBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-02T05:00:33.249383Z","bundle_sha256":"f5694a267f56573631b4fbe4792e51ae92771b4fb32fe3907185886124fcb655"}}