{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:RYSTNBGXC3RH3DQ33UJWEHKBLH","short_pith_number":"pith:RYSTNBGX","schema_version":"1.0","canonical_sha256":"8e253684d716e27d8e1bdd13621d4159edd38a92065b7f8f36fdebaee8a941d0","source":{"kind":"arxiv","id":"1504.07835","version":3},"attestation_state":"computed","paper":{"title":"Dynamo Effects Near The Transition from Solar to Anti-Solar Differential Rotation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.flu-dyn"],"primary_cat":"astro-ph.SR","authors_text":"Alexander G. Kosovichev, Friedrich H. Busse, Radostin D. Simitev","submitted_at":"2015-04-29T12:43:04Z","abstract_excerpt":"Numerical MHD simulations play increasingly important role for understanding mechanisms of stellar magnetism. We present simulations of convection and dynamos in density-stratified rotating spherical fluid shells. We employ a new 3D simulation code for the solution of a physically consistent anelastic model of the process with a minimum number of parameters. The reported dynamo simulations extend into a \"buoyancy-dominated\" regime where the buoyancy forcing is dominant while the Coriolis force is no longer balanced by pressure gradients and strong anti-solar differential rotation develops as a"},"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":"1504.07835","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-04-29T12:43:04Z","cross_cats_sorted":["physics.flu-dyn"],"title_canon_sha256":"f93140bba82bcfa0177bcc3e8dbddbdf35fc4b095166648ba0c36a85f7701670","abstract_canon_sha256":"becb104437a3d8bb87b2b5ee8a4598b49ba93b4ec221ccd55cbd00f7a5678e7f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:34:12.844390Z","signature_b64":"rznkO0KuFxcyusAHN/mQqle4Jx1Jlp1Jxkq1sGfegNI1haQfGx6DwtwfDdNPufk8HTomU6NoPgPtyqhwfjRbAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8e253684d716e27d8e1bdd13621d4159edd38a92065b7f8f36fdebaee8a941d0","last_reissued_at":"2026-05-18T01:34:12.843652Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:34:12.843652Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamo Effects Near The Transition from Solar to Anti-Solar Differential Rotation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.flu-dyn"],"primary_cat":"astro-ph.SR","authors_text":"Alexander G. Kosovichev, Friedrich H. Busse, Radostin D. Simitev","submitted_at":"2015-04-29T12:43:04Z","abstract_excerpt":"Numerical MHD simulations play increasingly important role for understanding mechanisms of stellar magnetism. We present simulations of convection and dynamos in density-stratified rotating spherical fluid shells. We employ a new 3D simulation code for the solution of a physically consistent anelastic model of the process with a minimum number of parameters. The reported dynamo simulations extend into a \"buoyancy-dominated\" regime where the buoyancy forcing is dominant while the Coriolis force is no longer balanced by pressure gradients and strong anti-solar differential rotation develops as a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.07835","kind":"arxiv","version":3},"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":"1504.07835","created_at":"2026-05-18T01:34:12.843747+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.07835v3","created_at":"2026-05-18T01:34:12.843747+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.07835","created_at":"2026-05-18T01:34:12.843747+00:00"},{"alias_kind":"pith_short_12","alias_value":"RYSTNBGXC3RH","created_at":"2026-05-18T12:29:39.896362+00:00"},{"alias_kind":"pith_short_16","alias_value":"RYSTNBGXC3RH3DQ3","created_at":"2026-05-18T12:29:39.896362+00:00"},{"alias_kind":"pith_short_8","alias_value":"RYSTNBGX","created_at":"2026-05-18T12:29:39.896362+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/RYSTNBGXC3RH3DQ33UJWEHKBLH","json":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH.json","graph_json":"https://pith.science/api/pith-number/RYSTNBGXC3RH3DQ33UJWEHKBLH/graph.json","events_json":"https://pith.science/api/pith-number/RYSTNBGXC3RH3DQ33UJWEHKBLH/events.json","paper":"https://pith.science/paper/RYSTNBGX"},"agent_actions":{"view_html":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH","download_json":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH.json","view_paper":"https://pith.science/paper/RYSTNBGX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.07835&json=true","fetch_graph":"https://pith.science/api/pith-number/RYSTNBGXC3RH3DQ33UJWEHKBLH/graph.json","fetch_events":"https://pith.science/api/pith-number/RYSTNBGXC3RH3DQ33UJWEHKBLH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH/action/storage_attestation","attest_author":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH/action/author_attestation","sign_citation":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH/action/citation_signature","submit_replication":"https://pith.science/pith/RYSTNBGXC3RH3DQ33UJWEHKBLH/action/replication_record"}},"created_at":"2026-05-18T01:34:12.843747+00:00","updated_at":"2026-05-18T01:34:12.843747+00:00"}