{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:JGFLNQV2YXUIKABDEBQ3RRHPPC","short_pith_number":"pith:JGFLNQV2","canonical_record":{"source":{"id":"1811.10534","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-11-20T21:51:44Z","cross_cats_sorted":["physics.flu-dyn"],"title_canon_sha256":"dc771260b85c8744eea292c4468d0445e1362ac0afe4454e2f331350d20e60d1","abstract_canon_sha256":"e5c11a8e489a900cf14da566ff3fc85a3ddfd1a4997b0d12810baaa3c779d5bd"},"schema_version":"1.0"},"canonical_sha256":"498ab6c2bac5e88500232061b8c4ef78b7bb115f10bc3043d81f778f73705291","source":{"kind":"arxiv","id":"1811.10534","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1811.10534","created_at":"2026-05-17T23:45:32Z"},{"alias_kind":"arxiv_version","alias_value":"1811.10534v1","created_at":"2026-05-17T23:45:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.10534","created_at":"2026-05-17T23:45:32Z"},{"alias_kind":"pith_short_12","alias_value":"JGFLNQV2YXUI","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JGFLNQV2YXUIKABD","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JGFLNQV2","created_at":"2026-05-18T12:32:31Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:JGFLNQV2YXUIKABDEBQ3RRHPPC","target":"record","payload":{"canonical_record":{"source":{"id":"1811.10534","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-11-20T21:51:44Z","cross_cats_sorted":["physics.flu-dyn"],"title_canon_sha256":"dc771260b85c8744eea292c4468d0445e1362ac0afe4454e2f331350d20e60d1","abstract_canon_sha256":"e5c11a8e489a900cf14da566ff3fc85a3ddfd1a4997b0d12810baaa3c779d5bd"},"schema_version":"1.0"},"canonical_sha256":"498ab6c2bac5e88500232061b8c4ef78b7bb115f10bc3043d81f778f73705291","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:45:32.737792Z","signature_b64":"zyxZfL7ze7/dvFIto6KowRZbOwcOx7af6ET+O5oHpRUuGJ3Pxyjp72XZbG36rW4oBZj+TXpYoh2Q6UAJPisQCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"498ab6c2bac5e88500232061b8c4ef78b7bb115f10bc3043d81f778f73705291","last_reissued_at":"2026-05-17T23:45:32.737092Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:45:32.737092Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1811.10534","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":"2026-05-17T23:45:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8/rfPvDimPmaVxeArYFF1bnkdEhdg5tNXTq06uQkA3UJ1W9SYjfmNy2a3GClLK0dN0qktnbfVQL35l5WA1iSDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:40:52.232410Z"},"content_sha256":"535273030c68248e2578cffb21689c3ab53e324c05e94b0697a46115c041ea16","schema_version":"1.0","event_id":"sha256:535273030c68248e2578cffb21689c3ab53e324c05e94b0697a46115c041ea16"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:JGFLNQV2YXUIKABDEBQ3RRHPPC","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Transition from weak to strong turbulence in magnetized plasmas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.flu-dyn"],"primary_cat":"physics.plasm-ph","authors_text":"David Hatch, Swadesh Mahajan, Vasil Bratanov","submitted_at":"2018-11-20T21:51:44Z","abstract_excerpt":"The scaling of turbulent heat flux with respect to electrostatic potential is examined in the framework of a reduced ($4$D) kinetic system describing electrostatic turbulence in magnetized plasmas excited by the ion temperature gradient instability. Numerical simulations were instigated by, and tested the predictions of generic renormalized turbulence models like the $2$D fluid model for electrostatic turbulence [Y.~Z.~Zhang and S.~M.~Mahajan, Phys.~Fluids B 5 (7), pp.~2000 (1993)]. A fundamental, perhaps, universal result of this theory-simulation combination is the demonstration that there e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.10534","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":"2026-05-17T23:45:32Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"6fL7mdR06Cnd85Y7I/yNi0fLmIArQ32llFivFA8SEToMTut/ekOCQKp+ylyTOQg6mrQ0vbZbG2uNOrUDP09WAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:40:52.233086Z"},"content_sha256":"4aa99344ad2cbc4897bd0fd1e5c1708338ce5826553970abdef959964d39dfe8","schema_version":"1.0","event_id":"sha256:4aa99344ad2cbc4897bd0fd1e5c1708338ce5826553970abdef959964d39dfe8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/JGFLNQV2YXUIKABDEBQ3RRHPPC/bundle.json","state_url":"https://pith.science/pith/JGFLNQV2YXUIKABDEBQ3RRHPPC/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/JGFLNQV2YXUIKABDEBQ3RRHPPC/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":"2026-05-25T17:40:52Z","links":{"resolver":"https://pith.science/pith/JGFLNQV2YXUIKABDEBQ3RRHPPC","bundle":"https://pith.science/pith/JGFLNQV2YXUIKABDEBQ3RRHPPC/bundle.json","state":"https://pith.science/pith/JGFLNQV2YXUIKABDEBQ3RRHPPC/state.json","well_known_bundle":"https://pith.science/.well-known/pith/JGFLNQV2YXUIKABDEBQ3RRHPPC/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:JGFLNQV2YXUIKABDEBQ3RRHPPC","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":"e5c11a8e489a900cf14da566ff3fc85a3ddfd1a4997b0d12810baaa3c779d5bd","cross_cats_sorted":["physics.flu-dyn"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-11-20T21:51:44Z","title_canon_sha256":"dc771260b85c8744eea292c4468d0445e1362ac0afe4454e2f331350d20e60d1"},"schema_version":"1.0","source":{"id":"1811.10534","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1811.10534","created_at":"2026-05-17T23:45:32Z"},{"alias_kind":"arxiv_version","alias_value":"1811.10534v1","created_at":"2026-05-17T23:45:32Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.10534","created_at":"2026-05-17T23:45:32Z"},{"alias_kind":"pith_short_12","alias_value":"JGFLNQV2YXUI","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_16","alias_value":"JGFLNQV2YXUIKABD","created_at":"2026-05-18T12:32:31Z"},{"alias_kind":"pith_short_8","alias_value":"JGFLNQV2","created_at":"2026-05-18T12:32:31Z"}],"graph_snapshots":[{"event_id":"sha256:4aa99344ad2cbc4897bd0fd1e5c1708338ce5826553970abdef959964d39dfe8","target":"graph","created_at":"2026-05-17T23:45:32Z","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":"The scaling of turbulent heat flux with respect to electrostatic potential is examined in the framework of a reduced ($4$D) kinetic system describing electrostatic turbulence in magnetized plasmas excited by the ion temperature gradient instability. Numerical simulations were instigated by, and tested the predictions of generic renormalized turbulence models like the $2$D fluid model for electrostatic turbulence [Y.~Z.~Zhang and S.~M.~Mahajan, Phys.~Fluids B 5 (7), pp.~2000 (1993)]. A fundamental, perhaps, universal result of this theory-simulation combination is the demonstration that there e","authors_text":"David Hatch, Swadesh Mahajan, Vasil Bratanov","cross_cats":["physics.flu-dyn"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-11-20T21:51:44Z","title":"Transition from weak to strong turbulence in magnetized plasmas"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.10534","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":"sha256:535273030c68248e2578cffb21689c3ab53e324c05e94b0697a46115c041ea16","target":"record","created_at":"2026-05-17T23:45:32Z","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":"e5c11a8e489a900cf14da566ff3fc85a3ddfd1a4997b0d12810baaa3c779d5bd","cross_cats_sorted":["physics.flu-dyn"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-11-20T21:51:44Z","title_canon_sha256":"dc771260b85c8744eea292c4468d0445e1362ac0afe4454e2f331350d20e60d1"},"schema_version":"1.0","source":{"id":"1811.10534","kind":"arxiv","version":1}},"canonical_sha256":"498ab6c2bac5e88500232061b8c4ef78b7bb115f10bc3043d81f778f73705291","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"498ab6c2bac5e88500232061b8c4ef78b7bb115f10bc3043d81f778f73705291","first_computed_at":"2026-05-17T23:45:32.737092Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:45:32.737092Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"zyxZfL7ze7/dvFIto6KowRZbOwcOx7af6ET+O5oHpRUuGJ3Pxyjp72XZbG36rW4oBZj+TXpYoh2Q6UAJPisQCQ==","signature_status":"signed_v1","signed_at":"2026-05-17T23:45:32.737792Z","signed_message":"canonical_sha256_bytes"},"source_id":"1811.10534","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:535273030c68248e2578cffb21689c3ab53e324c05e94b0697a46115c041ea16","sha256:4aa99344ad2cbc4897bd0fd1e5c1708338ce5826553970abdef959964d39dfe8"],"state_sha256":"8612d4d4c9f092d7ce2f5b8922c389e4124eedfadece3f7f20f49c9ac8e09580"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"NDDzCSGjvsKyTU1nGLYfX4hAqiydgHwEAdaEDpawTPO85wbD2tbyBVCNj/Rzp3HacqPD+5JzPT9ORloQuA6rAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T17:40:52.236802Z","bundle_sha256":"12f1bb10a525dead4da9950b70b2f0d0433f78e5edab8e8491bbb451cb96ae25"}}