{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:I4UEHGXDWYCOA2TJ3AWC53ZUO3","short_pith_number":"pith:I4UEHGXD","schema_version":"1.0","canonical_sha256":"4728439ae3b604e06a69d82c2eef3476c2979683d5d517e2ef500d64d8658e98","source":{"kind":"arxiv","id":"1510.04178","version":1},"attestation_state":"computed","paper":{"title":"Dynamo saturation in direct simulations of the multi-phase turbulent interstellar medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bendre, D. Elstner, O. Gressel","submitted_at":"2015-10-14T15:59:38Z","abstract_excerpt":"The ordered magnetic field observed via polarized synchrotron emission in nearby disc galaxies can be explained by a mean-field dynamo operating in the diffuse interstellar medium (ISM). Additionally, vertical-flux initial conditions are potentially able to influence this dynamo via the occurrence of the magneto-rotational instability (MRI). We aim to study the influence of various initial field configurations on the saturated state of the mean-field dynamo. This is motivated by the observation that different saturation behavior was previously obtained for different supernova rates. We perform"},"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":"1510.04178","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-10-14T15:59:38Z","cross_cats_sorted":[],"title_canon_sha256":"7f96b9cc37a6baa5921cdf1d645a5a41be2485601c7e2b1e03dd2953b9e0110d","abstract_canon_sha256":"a83ae1cbb4f5218991763c2cf69417f11713d8aef0a20e2337458a305c2ab249"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:22.904108Z","signature_b64":"DYN3r5XrfX3oolAsHIzy6gGoxD/JTKFstBRfzS2/fGtLLgkisXZEvw+58juVesHBPjsxaqNZQOKEA5YgUWZFAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4728439ae3b604e06a69d82c2eef3476c2979683d5d517e2ef500d64d8658e98","last_reissued_at":"2026-05-18T01:23:22.903421Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:22.903421Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamo saturation in direct simulations of the multi-phase turbulent interstellar medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bendre, D. Elstner, O. Gressel","submitted_at":"2015-10-14T15:59:38Z","abstract_excerpt":"The ordered magnetic field observed via polarized synchrotron emission in nearby disc galaxies can be explained by a mean-field dynamo operating in the diffuse interstellar medium (ISM). Additionally, vertical-flux initial conditions are potentially able to influence this dynamo via the occurrence of the magneto-rotational instability (MRI). We aim to study the influence of various initial field configurations on the saturated state of the mean-field dynamo. This is motivated by the observation that different saturation behavior was previously obtained for different supernova rates. We perform"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.04178","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":"1510.04178","created_at":"2026-05-18T01:23:22.903533+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.04178v1","created_at":"2026-05-18T01:23:22.903533+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.04178","created_at":"2026-05-18T01:23:22.903533+00:00"},{"alias_kind":"pith_short_12","alias_value":"I4UEHGXDWYCO","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_16","alias_value":"I4UEHGXDWYCOA2TJ","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_8","alias_value":"I4UEHGXD","created_at":"2026-05-18T12:29:25.134429+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/I4UEHGXDWYCOA2TJ3AWC53ZUO3","json":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3.json","graph_json":"https://pith.science/api/pith-number/I4UEHGXDWYCOA2TJ3AWC53ZUO3/graph.json","events_json":"https://pith.science/api/pith-number/I4UEHGXDWYCOA2TJ3AWC53ZUO3/events.json","paper":"https://pith.science/paper/I4UEHGXD"},"agent_actions":{"view_html":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3","download_json":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3.json","view_paper":"https://pith.science/paper/I4UEHGXD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.04178&json=true","fetch_graph":"https://pith.science/api/pith-number/I4UEHGXDWYCOA2TJ3AWC53ZUO3/graph.json","fetch_events":"https://pith.science/api/pith-number/I4UEHGXDWYCOA2TJ3AWC53ZUO3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3/action/storage_attestation","attest_author":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3/action/author_attestation","sign_citation":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3/action/citation_signature","submit_replication":"https://pith.science/pith/I4UEHGXDWYCOA2TJ3AWC53ZUO3/action/replication_record"}},"created_at":"2026-05-18T01:23:22.903533+00:00","updated_at":"2026-05-18T01:23:22.903533+00:00"}