{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:5WNJDXWKYPDU5RYXHL6WEYAJB4","short_pith_number":"pith:5WNJDXWK","schema_version":"1.0","canonical_sha256":"ed9a91decac3c74ec7173afd6260090f38858f1fa7dde305437d27e8bddea882","source":{"kind":"arxiv","id":"1710.03174","version":2},"attestation_state":"computed","paper":{"title":"Large-scale dynamos in rapidly rotating plane layer convection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","physics.flu-dyn"],"primary_cat":"astro-ph.SR","authors_text":"A. Brandenburg, B. Favier, C. Guervilly, M. J. K\\\"apyl\\\"a, P. J. Bushby, P. J. K\\\"apyl\\\"a, Y. Masada","submitted_at":"2017-10-09T16:20:09Z","abstract_excerpt":"Context: Convectively-driven flows play a crucial role in the dynamo processes that are responsible for producing magnetic activity in stars and planets. It is still not fully understood why many astrophysical magnetic fields have a significant large-scale component. Aims: Our aim is to investigate the dynamo properties of compressible convection in a rapidly rotating Cartesian domain, focusing upon a parameter regime in which the underlying hydrodynamic flow is known to be unstable to a large-scale vortex instability. Methods: The governing equations of three-dimensional nonlinear magnetohydr"},"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":"1710.03174","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-10-09T16:20:09Z","cross_cats_sorted":["astro-ph.EP","physics.flu-dyn"],"title_canon_sha256":"667c30ea9d78b86139bb39c4aa5611a5427345075af76bc0903e780076d923f2","abstract_canon_sha256":"c428adc4c6413df6c615003a988b2988aebb8fa6252c9272a268a3870f7d4d82"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:16:30.983736Z","signature_b64":"1YenBXlu3vIb+0kKbprj6fORj41OOxJISvgfq4XStwT1odE79dMtcnah1yYv6UvMfx5GRcDvbLZW9rnV+w+CDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ed9a91decac3c74ec7173afd6260090f38858f1fa7dde305437d27e8bddea882","last_reissued_at":"2026-05-18T00:16:30.983071Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:16:30.983071Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Large-scale dynamos in rapidly rotating plane layer convection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","physics.flu-dyn"],"primary_cat":"astro-ph.SR","authors_text":"A. Brandenburg, B. Favier, C. Guervilly, M. J. K\\\"apyl\\\"a, P. J. Bushby, P. J. K\\\"apyl\\\"a, Y. Masada","submitted_at":"2017-10-09T16:20:09Z","abstract_excerpt":"Context: Convectively-driven flows play a crucial role in the dynamo processes that are responsible for producing magnetic activity in stars and planets. It is still not fully understood why many astrophysical magnetic fields have a significant large-scale component. Aims: Our aim is to investigate the dynamo properties of compressible convection in a rapidly rotating Cartesian domain, focusing upon a parameter regime in which the underlying hydrodynamic flow is known to be unstable to a large-scale vortex instability. Methods: The governing equations of three-dimensional nonlinear magnetohydr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.03174","kind":"arxiv","version":2},"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":"1710.03174","created_at":"2026-05-18T00:16:30.983170+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.03174v2","created_at":"2026-05-18T00:16:30.983170+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.03174","created_at":"2026-05-18T00:16:30.983170+00:00"},{"alias_kind":"pith_short_12","alias_value":"5WNJDXWKYPDU","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_16","alias_value":"5WNJDXWKYPDU5RYX","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_8","alias_value":"5WNJDXWK","created_at":"2026-05-18T12:31:03.183658+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/5WNJDXWKYPDU5RYXHL6WEYAJB4","json":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4.json","graph_json":"https://pith.science/api/pith-number/5WNJDXWKYPDU5RYXHL6WEYAJB4/graph.json","events_json":"https://pith.science/api/pith-number/5WNJDXWKYPDU5RYXHL6WEYAJB4/events.json","paper":"https://pith.science/paper/5WNJDXWK"},"agent_actions":{"view_html":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4","download_json":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4.json","view_paper":"https://pith.science/paper/5WNJDXWK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.03174&json=true","fetch_graph":"https://pith.science/api/pith-number/5WNJDXWKYPDU5RYXHL6WEYAJB4/graph.json","fetch_events":"https://pith.science/api/pith-number/5WNJDXWKYPDU5RYXHL6WEYAJB4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4/action/storage_attestation","attest_author":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4/action/author_attestation","sign_citation":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4/action/citation_signature","submit_replication":"https://pith.science/pith/5WNJDXWKYPDU5RYXHL6WEYAJB4/action/replication_record"}},"created_at":"2026-05-18T00:16:30.983170+00:00","updated_at":"2026-05-18T00:16:30.983170+00:00"}