{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:RVE443DIQZMEX6DOPBEY2MGCOO","short_pith_number":"pith:RVE443DI","schema_version":"1.0","canonical_sha256":"8d49ce6c6886584bf86e78498d30c273b37db478c0adb73fc8dd11a9c51d9816","source":{"kind":"arxiv","id":"1301.7508","version":1},"attestation_state":"computed","paper":{"title":"Characterizing Magnetized Turbulence in M51","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Andrew Fletcher, Jeroen M. Stil, John E. Vaillancourt, Martin Houde, Rainer Beck, Roger H. Hildebrand","submitted_at":"2013-01-31T04:08:16Z","abstract_excerpt":"We use previously published high-resolution synchrotron polarization data to perform an angular dispersion analysis with the aim of charactering magnetized turbulence in M51. We first analyze three distinct regions (the center of the galaxy, and the northwest and southwest spiral arms) and can clearly discern the turbulent correlation length scale from the width of the magnetized turbulent correlation function for two regions and detect the imprint of anisotropy in the turbulence for all three. Furthermore, analyzing the galaxy as a whole allows us to determine a two-dimensional Gaussian model"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1301.7508","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-01-31T04:08:16Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"635aa425b108938b979c6fa402ddae24c6b873139e7b38245db9309ec009c529","abstract_canon_sha256":"b31aa0b21757455a5dc9ac77ed3fdad575877fe8b01a7ec2c267977ee31044d3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:56.779693Z","signature_b64":"AZw342mnfBcwq8TYPmYN02cqZSvtIyVcPferwXXHEa9Vl1hFMsPcdXP8K+mZYSj3RgGEa/AMQsQyFD7USP/fAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8d49ce6c6886584bf86e78498d30c273b37db478c0adb73fc8dd11a9c51d9816","last_reissued_at":"2026-05-18T01:51:56.779234Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:56.779234Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Characterizing Magnetized Turbulence in M51","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Andrew Fletcher, Jeroen M. Stil, John E. Vaillancourt, Martin Houde, Rainer Beck, Roger H. Hildebrand","submitted_at":"2013-01-31T04:08:16Z","abstract_excerpt":"We use previously published high-resolution synchrotron polarization data to perform an angular dispersion analysis with the aim of charactering magnetized turbulence in M51. We first analyze three distinct regions (the center of the galaxy, and the northwest and southwest spiral arms) and can clearly discern the turbulent correlation length scale from the width of the magnetized turbulent correlation function for two regions and detect the imprint of anisotropy in the turbulence for all three. Furthermore, analyzing the galaxy as a whole allows us to determine a two-dimensional Gaussian model"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.7508","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1301.7508","created_at":"2026-05-18T01:51:56.779310+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.7508v1","created_at":"2026-05-18T01:51:56.779310+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.7508","created_at":"2026-05-18T01:51:56.779310+00:00"},{"alias_kind":"pith_short_12","alias_value":"RVE443DIQZME","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"RVE443DIQZMEX6DO","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"RVE443DI","created_at":"2026-05-18T12:27:59.945178+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO","json":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO.json","graph_json":"https://pith.science/api/pith-number/RVE443DIQZMEX6DOPBEY2MGCOO/graph.json","events_json":"https://pith.science/api/pith-number/RVE443DIQZMEX6DOPBEY2MGCOO/events.json","paper":"https://pith.science/paper/RVE443DI"},"agent_actions":{"view_html":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO","download_json":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO.json","view_paper":"https://pith.science/paper/RVE443DI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.7508&json=true","fetch_graph":"https://pith.science/api/pith-number/RVE443DIQZMEX6DOPBEY2MGCOO/graph.json","fetch_events":"https://pith.science/api/pith-number/RVE443DIQZMEX6DOPBEY2MGCOO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO/action/storage_attestation","attest_author":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO/action/author_attestation","sign_citation":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO/action/citation_signature","submit_replication":"https://pith.science/pith/RVE443DIQZMEX6DOPBEY2MGCOO/action/replication_record"}},"created_at":"2026-05-18T01:51:56.779310+00:00","updated_at":"2026-05-18T01:51:56.779310+00:00"}