{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:EMMRM5D5SSSAETWDQGAJ7QJKJ6","short_pith_number":"pith:EMMRM5D5","canonical_record":{"source":{"id":"1002.2096","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2010-02-10T14:05:17Z","cross_cats_sorted":["astro-ph.SR","physics.flu-dyn","physics.plasm-ph"],"title_canon_sha256":"8e04995bc6838c295d0ffa27d58d957e0fcb5187b2b2612596e1db615cbf7f83","abstract_canon_sha256":"cd2803cf1153e5e5e0514b7a0ad3912973ab7141d597f98048a80173afa542ad"},"schema_version":"1.0"},"canonical_sha256":"231916747d94a4024ec381809fc12a4f9346655e153fc65f6e557e9517dc3644","source":{"kind":"arxiv","id":"1002.2096","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1002.2096","created_at":"2026-05-18T02:09:10Z"},{"alias_kind":"arxiv_version","alias_value":"1002.2096v1","created_at":"2026-05-18T02:09:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1002.2096","created_at":"2026-05-18T02:09:10Z"},{"alias_kind":"pith_short_12","alias_value":"EMMRM5D5SSSA","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"EMMRM5D5SSSAETWD","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"EMMRM5D5","created_at":"2026-05-18T12:26:06Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:EMMRM5D5SSSAETWDQGAJ7QJKJ6","target":"record","payload":{"canonical_record":{"source":{"id":"1002.2096","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2010-02-10T14:05:17Z","cross_cats_sorted":["astro-ph.SR","physics.flu-dyn","physics.plasm-ph"],"title_canon_sha256":"8e04995bc6838c295d0ffa27d58d957e0fcb5187b2b2612596e1db615cbf7f83","abstract_canon_sha256":"cd2803cf1153e5e5e0514b7a0ad3912973ab7141d597f98048a80173afa542ad"},"schema_version":"1.0"},"canonical_sha256":"231916747d94a4024ec381809fc12a4f9346655e153fc65f6e557e9517dc3644","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:09:10.221183Z","signature_b64":"i6l99XQ1mT2Vdgk7nipnHk8LzKIR6rHaRgxvE3UpNsETDYhmuOaGsCv+kPIjvIQhuDB29E5JkQwvtRwb10YHCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"231916747d94a4024ec381809fc12a4f9346655e153fc65f6e557e9517dc3644","last_reissued_at":"2026-05-18T02:09:10.220444Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:09:10.220444Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1002.2096","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":"2026-05-18T02:09:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"9g4hLMxTRNeD1HxEeAnHs+aJo2abuVCHQklRRCkoHhU34u55lULC7rxR1RlXBaGzSSEPfXG5wcwyVkfvDlNFAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T10:07:00.406894Z"},"content_sha256":"58e8459d417188b5706b043f0bcdbb13938ac292e08378100f2192cb75179196","schema_version":"1.0","event_id":"sha256:58e8459d417188b5706b043f0bcdbb13938ac292e08378100f2192cb75179196"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:EMMRM5D5SSSAETWDQGAJ7QJKJ6","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Power and spectral index anisotropy of the entire inertial range of turbulence in the fast solar wind","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.flu-dyn","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"A. A. Schekochihin, C. H. K. Chen, R. T. Wicks, T. S. Horbury","submitted_at":"2010-02-10T14:05:17Z","abstract_excerpt":"We measure the power and spectral index anisotropy of high speed solar wind turbulence from scales larger than the outer scale down to the ion gyroscale, thus covering the entire inertial range. We show that the power and spectral indices at the outer scale of turbulence are approximately isotropic. The turbulent cascade causes the power anisotropy at smaller scales manifested by anisotropic scalings of the spectrum: close to k^{-5/3} across and k^{-2} along the local magnetic field, consistent with a critically balanced Alfvenic turbulence. By using data at different radial distances from the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1002.2096","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":"2026-05-18T02:09:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"xT41npilfqYVcs9e9MUT+sn/2RM4KrB0xXb1U4KRBbUEU3rbcWUv1v/6vyQETmLiGd8vn/OS+SNz6JL7aP0DDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T10:07:00.407267Z"},"content_sha256":"0e45839b7c93a728f9dc6f546fe97c16e241dcb94101f9da2ebb9327c4443a7f","schema_version":"1.0","event_id":"sha256:0e45839b7c93a728f9dc6f546fe97c16e241dcb94101f9da2ebb9327c4443a7f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/EMMRM5D5SSSAETWDQGAJ7QJKJ6/bundle.json","state_url":"https://pith.science/pith/EMMRM5D5SSSAETWDQGAJ7QJKJ6/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/EMMRM5D5SSSAETWDQGAJ7QJKJ6/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":"2026-05-25T10:07:00Z","links":{"resolver":"https://pith.science/pith/EMMRM5D5SSSAETWDQGAJ7QJKJ6","bundle":"https://pith.science/pith/EMMRM5D5SSSAETWDQGAJ7QJKJ6/bundle.json","state":"https://pith.science/pith/EMMRM5D5SSSAETWDQGAJ7QJKJ6/state.json","well_known_bundle":"https://pith.science/.well-known/pith/EMMRM5D5SSSAETWDQGAJ7QJKJ6/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:EMMRM5D5SSSAETWDQGAJ7QJKJ6","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":"cd2803cf1153e5e5e0514b7a0ad3912973ab7141d597f98048a80173afa542ad","cross_cats_sorted":["astro-ph.SR","physics.flu-dyn","physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2010-02-10T14:05:17Z","title_canon_sha256":"8e04995bc6838c295d0ffa27d58d957e0fcb5187b2b2612596e1db615cbf7f83"},"schema_version":"1.0","source":{"id":"1002.2096","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1002.2096","created_at":"2026-05-18T02:09:10Z"},{"alias_kind":"arxiv_version","alias_value":"1002.2096v1","created_at":"2026-05-18T02:09:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1002.2096","created_at":"2026-05-18T02:09:10Z"},{"alias_kind":"pith_short_12","alias_value":"EMMRM5D5SSSA","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_16","alias_value":"EMMRM5D5SSSAETWD","created_at":"2026-05-18T12:26:06Z"},{"alias_kind":"pith_short_8","alias_value":"EMMRM5D5","created_at":"2026-05-18T12:26:06Z"}],"graph_snapshots":[{"event_id":"sha256:0e45839b7c93a728f9dc6f546fe97c16e241dcb94101f9da2ebb9327c4443a7f","target":"graph","created_at":"2026-05-18T02:09:10Z","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 measure the power and spectral index anisotropy of high speed solar wind turbulence from scales larger than the outer scale down to the ion gyroscale, thus covering the entire inertial range. We show that the power and spectral indices at the outer scale of turbulence are approximately isotropic. The turbulent cascade causes the power anisotropy at smaller scales manifested by anisotropic scalings of the spectrum: close to k^{-5/3} across and k^{-2} along the local magnetic field, consistent with a critically balanced Alfvenic turbulence. By using data at different radial distances from the","authors_text":"A. A. Schekochihin, C. H. K. Chen, R. T. Wicks, T. S. Horbury","cross_cats":["astro-ph.SR","physics.flu-dyn","physics.plasm-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2010-02-10T14:05:17Z","title":"Power and spectral index anisotropy of the entire inertial range of turbulence in the fast solar wind"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1002.2096","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":"sha256:58e8459d417188b5706b043f0bcdbb13938ac292e08378100f2192cb75179196","target":"record","created_at":"2026-05-18T02:09:10Z","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":"cd2803cf1153e5e5e0514b7a0ad3912973ab7141d597f98048a80173afa542ad","cross_cats_sorted":["astro-ph.SR","physics.flu-dyn","physics.plasm-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.space-ph","submitted_at":"2010-02-10T14:05:17Z","title_canon_sha256":"8e04995bc6838c295d0ffa27d58d957e0fcb5187b2b2612596e1db615cbf7f83"},"schema_version":"1.0","source":{"id":"1002.2096","kind":"arxiv","version":1}},"canonical_sha256":"231916747d94a4024ec381809fc12a4f9346655e153fc65f6e557e9517dc3644","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"231916747d94a4024ec381809fc12a4f9346655e153fc65f6e557e9517dc3644","first_computed_at":"2026-05-18T02:09:10.220444Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:09:10.220444Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"i6l99XQ1mT2Vdgk7nipnHk8LzKIR6rHaRgxvE3UpNsETDYhmuOaGsCv+kPIjvIQhuDB29E5JkQwvtRwb10YHCg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:09:10.221183Z","signed_message":"canonical_sha256_bytes"},"source_id":"1002.2096","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:58e8459d417188b5706b043f0bcdbb13938ac292e08378100f2192cb75179196","sha256:0e45839b7c93a728f9dc6f546fe97c16e241dcb94101f9da2ebb9327c4443a7f"],"state_sha256":"ea5c20ea1eeef2b8b45bb102d2bb426efbd93d70c37bd01ee442a35eeaa521f8"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"wai1PRTLou4jAN+w2VifKFCCBEpXPNUT5IiQq8H34j7otZ8X158a2fVi8JDA4+caMnzDs2E4tdyJne4qwSjQDA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T10:07:00.409773Z","bundle_sha256":"aa3b8f4e086feef035433ecac4ddac6b158446e68c1c504b2a08d456f802ce30"}}