{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QEE3RSCGJMCQZM4QCYKU5UGVA6","short_pith_number":"pith:QEE3RSCG","schema_version":"1.0","canonical_sha256":"8109b8c8464b050cb39016154ed0d5079ac1350a395789d887c38aba2a2bc833","source":{"kind":"arxiv","id":"1610.07634","version":2},"attestation_state":"computed","paper":{"title":"Kinematics of Magnetic Bright Features in the Solar Photosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Gandorfer, D. Orozco Suarez, J. Blanco Rodriguez, J. C. del Toro Iniesta, J. Hirzberger, L. Gizon, M. Knoelker, M. van Noort, P. Barthol, R. H. Cameron, Shahin Jafarzadeh, S. K. Solanki, T. L. Riethmueller, V. Martinez Pillet, W. Schmidt","submitted_at":"2016-10-24T20:19:48Z","abstract_excerpt":"Convective flows are known as the prime means of transporting magnetic fields on the solar surface. Thus, small magnetic structures are good tracers of the turbulent flows. We study the migration and dispersal of magnetic bright features (MBFs) in intergranular areas observed at high spatial resolution with Sunrise/IMaX. We describe the flux dispersal of individual MBFs as a diffusion process whose parameters are computed for various areas in the quiet Sun and the vicinity of active regions from seeing-free data. We find that magnetic concentrations are best described as random walkers close t"},"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":"1610.07634","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-24T20:19:48Z","cross_cats_sorted":[],"title_canon_sha256":"3764db2537c5d14134858aac24db320e2b9fd033d9b22b233c96655cfdc1bbed","abstract_canon_sha256":"931ec7b94f14d2e1a072f05670cdeaa8d83f59a7b135b77fb9307e5e1c2925d2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:47:42.636452Z","signature_b64":"2C2eXHl6H5caPMK9ibbce2zl5bnz8Az6qvk7PlAtaCXo3f8binyCrgtgODDzd7A70Wf3VUrd/XYadLVgItGPDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8109b8c8464b050cb39016154ed0d5079ac1350a395789d887c38aba2a2bc833","last_reissued_at":"2026-05-18T00:47:42.635947Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:47:42.635947Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinematics of Magnetic Bright Features in the Solar Photosphere","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Gandorfer, D. Orozco Suarez, J. Blanco Rodriguez, J. C. del Toro Iniesta, J. Hirzberger, L. Gizon, M. Knoelker, M. van Noort, P. Barthol, R. H. Cameron, Shahin Jafarzadeh, S. K. Solanki, T. L. Riethmueller, V. Martinez Pillet, W. Schmidt","submitted_at":"2016-10-24T20:19:48Z","abstract_excerpt":"Convective flows are known as the prime means of transporting magnetic fields on the solar surface. Thus, small magnetic structures are good tracers of the turbulent flows. We study the migration and dispersal of magnetic bright features (MBFs) in intergranular areas observed at high spatial resolution with Sunrise/IMaX. We describe the flux dispersal of individual MBFs as a diffusion process whose parameters are computed for various areas in the quiet Sun and the vicinity of active regions from seeing-free data. We find that magnetic concentrations are best described as random walkers close t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.07634","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":"1610.07634","created_at":"2026-05-18T00:47:42.636020+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.07634v2","created_at":"2026-05-18T00:47:42.636020+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.07634","created_at":"2026-05-18T00:47:42.636020+00:00"},{"alias_kind":"pith_short_12","alias_value":"QEE3RSCGJMCQ","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"QEE3RSCGJMCQZM4Q","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"QEE3RSCG","created_at":"2026-05-18T12:30:39.010887+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/QEE3RSCGJMCQZM4QCYKU5UGVA6","json":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6.json","graph_json":"https://pith.science/api/pith-number/QEE3RSCGJMCQZM4QCYKU5UGVA6/graph.json","events_json":"https://pith.science/api/pith-number/QEE3RSCGJMCQZM4QCYKU5UGVA6/events.json","paper":"https://pith.science/paper/QEE3RSCG"},"agent_actions":{"view_html":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6","download_json":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6.json","view_paper":"https://pith.science/paper/QEE3RSCG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.07634&json=true","fetch_graph":"https://pith.science/api/pith-number/QEE3RSCGJMCQZM4QCYKU5UGVA6/graph.json","fetch_events":"https://pith.science/api/pith-number/QEE3RSCGJMCQZM4QCYKU5UGVA6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6/action/storage_attestation","attest_author":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6/action/author_attestation","sign_citation":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6/action/citation_signature","submit_replication":"https://pith.science/pith/QEE3RSCGJMCQZM4QCYKU5UGVA6/action/replication_record"}},"created_at":"2026-05-18T00:47:42.636020+00:00","updated_at":"2026-05-18T00:47:42.636020+00:00"}