{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:NEJHFA2QEDVKIIRUWO4VARSTJG","short_pith_number":"pith:NEJHFA2Q","schema_version":"1.0","canonical_sha256":"691272835020eaa42234b3b950465349a3b558e0dc5bda881cb532c3c2f3f9de","source":{"kind":"arxiv","id":"1811.05356","version":2},"attestation_state":"computed","paper":{"title":"The Solar Wind in Time II: 3D stellar wind structure and radio emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. A. Vidotto, C. P. Folsom, D. \\'O Fionnag\\'ain, J.-D. do Nascimento Jr, J. Morin, P. Petit, S. C. Marsden, S. V. Jeffers","submitted_at":"2018-11-13T15:06:29Z","abstract_excerpt":"In this work, we simulate the evolution of the solar wind along its main sequence lifetime and compute its thermal radio emission. To study the evolution of the solar wind, we use a sample of solar mass stars at different ages. All these stars have observationally-reconstructed magnetic maps, which are incorporated in our 3D magnetohydrodynamic simulations of their winds. We show that angular-momentum loss and mass-loss rates decrease steadily on evolutionary timescales, although they can vary in a magnetic cycle timescale. Stellar winds are known to emit radiation in the form of thermal brems"},"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":"1811.05356","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-11-13T15:06:29Z","cross_cats_sorted":[],"title_canon_sha256":"9f3fd9ba62a91d2abbea632a10eec3ba3a6867a312a6f561d085af3a2f95d490","abstract_canon_sha256":"d078ad9f1203e726d7de598b996dba023f626907bd3e75b708cfc8bc5e9ceab3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:43:23.492175Z","signature_b64":"6kup9MPXfGGSj2l2FJmOdJrnyJMfCS4zYdKJg+IWYo8+tLPrmnN9l/2mLBccUKNClsdr8x9voOxubHXiV1CFCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"691272835020eaa42234b3b950465349a3b558e0dc5bda881cb532c3c2f3f9de","last_reissued_at":"2026-05-17T23:43:23.491495Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:43:23.491495Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Solar Wind in Time II: 3D stellar wind structure and radio emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. A. Vidotto, C. P. Folsom, D. \\'O Fionnag\\'ain, J.-D. do Nascimento Jr, J. Morin, P. Petit, S. C. Marsden, S. V. Jeffers","submitted_at":"2018-11-13T15:06:29Z","abstract_excerpt":"In this work, we simulate the evolution of the solar wind along its main sequence lifetime and compute its thermal radio emission. To study the evolution of the solar wind, we use a sample of solar mass stars at different ages. All these stars have observationally-reconstructed magnetic maps, which are incorporated in our 3D magnetohydrodynamic simulations of their winds. We show that angular-momentum loss and mass-loss rates decrease steadily on evolutionary timescales, although they can vary in a magnetic cycle timescale. Stellar winds are known to emit radiation in the form of thermal brems"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.05356","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":"1811.05356","created_at":"2026-05-17T23:43:23.491599+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.05356v2","created_at":"2026-05-17T23:43:23.491599+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.05356","created_at":"2026-05-17T23:43:23.491599+00:00"},{"alias_kind":"pith_short_12","alias_value":"NEJHFA2QEDVK","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_16","alias_value":"NEJHFA2QEDVKIIRU","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_8","alias_value":"NEJHFA2Q","created_at":"2026-05-18T12:32:40.477152+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/NEJHFA2QEDVKIIRUWO4VARSTJG","json":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG.json","graph_json":"https://pith.science/api/pith-number/NEJHFA2QEDVKIIRUWO4VARSTJG/graph.json","events_json":"https://pith.science/api/pith-number/NEJHFA2QEDVKIIRUWO4VARSTJG/events.json","paper":"https://pith.science/paper/NEJHFA2Q"},"agent_actions":{"view_html":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG","download_json":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG.json","view_paper":"https://pith.science/paper/NEJHFA2Q","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.05356&json=true","fetch_graph":"https://pith.science/api/pith-number/NEJHFA2QEDVKIIRUWO4VARSTJG/graph.json","fetch_events":"https://pith.science/api/pith-number/NEJHFA2QEDVKIIRUWO4VARSTJG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG/action/storage_attestation","attest_author":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG/action/author_attestation","sign_citation":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG/action/citation_signature","submit_replication":"https://pith.science/pith/NEJHFA2QEDVKIIRUWO4VARSTJG/action/replication_record"}},"created_at":"2026-05-17T23:43:23.491599+00:00","updated_at":"2026-05-17T23:43:23.491599+00:00"}