{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:Y32RW23IYIMF5PTGNGZAV7DCFE","short_pith_number":"pith:Y32RW23I","schema_version":"1.0","canonical_sha256":"c6f51b6b68c2185ebe6669b20afc622907dd632dad86fb3fae0d66551d3f34b9","source":{"kind":"arxiv","id":"1710.02137","version":1},"attestation_state":"computed","paper":{"title":"Probing Subsurface Flows in Active Region NOAA 12192 - Comparison with NOAA 10486","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Hill, Kiran Jain, S.C. Tripathy","submitted_at":"2017-10-05T17:53:52Z","abstract_excerpt":"Active Region (AR) 12192 is the biggest AR observed in solar cycle 24 so far. This was a long-lived AR which survived for four Carrington rotations (CR) and exhibited several unusual phenomena. We measure the horizontal subsurface flows in this active region in multiple rotation using the ring-diagram technique of local helioseismology and the Global Oscillation Network Group (GONG+) Dopplergrams, and investigate how different was the plasma flow in AR 12192 from that in AR 10486. Both regions produced several high M- and X-class flares but had different CME productivity. Our analysis suggests"},"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":"1710.02137","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-10-05T17:53:52Z","cross_cats_sorted":[],"title_canon_sha256":"cd1b8453843a1fe254a35131efe47c87bd18cc56350cc76489a01ec1a600848c","abstract_canon_sha256":"8382e1ba1cda7053b21daddb19c3ea6137323dea2e05de8ad51534a9997a55fc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:30:40.745705Z","signature_b64":"grv+HJ1LZwtSP7Ib/x27I8V0xJmE6TFx0HTZY5FqRdV5RGnoxCLAtcosjXg+CIboIRxf5Ni2tLN4u29F38niAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c6f51b6b68c2185ebe6669b20afc622907dd632dad86fb3fae0d66551d3f34b9","last_reissued_at":"2026-05-18T00:30:40.745160Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:30:40.745160Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing Subsurface Flows in Active Region NOAA 12192 - Comparison with NOAA 10486","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Hill, Kiran Jain, S.C. Tripathy","submitted_at":"2017-10-05T17:53:52Z","abstract_excerpt":"Active Region (AR) 12192 is the biggest AR observed in solar cycle 24 so far. This was a long-lived AR which survived for four Carrington rotations (CR) and exhibited several unusual phenomena. We measure the horizontal subsurface flows in this active region in multiple rotation using the ring-diagram technique of local helioseismology and the Global Oscillation Network Group (GONG+) Dopplergrams, and investigate how different was the plasma flow in AR 12192 from that in AR 10486. Both regions produced several high M- and X-class flares but had different CME productivity. Our analysis suggests"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.02137","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":"1710.02137","created_at":"2026-05-18T00:30:40.745243+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.02137v1","created_at":"2026-05-18T00:30:40.745243+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.02137","created_at":"2026-05-18T00:30:40.745243+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y32RW23IYIMF","created_at":"2026-05-18T12:31:56.362134+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y32RW23IYIMF5PTG","created_at":"2026-05-18T12:31:56.362134+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y32RW23I","created_at":"2026-05-18T12:31:56.362134+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/Y32RW23IYIMF5PTGNGZAV7DCFE","json":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE.json","graph_json":"https://pith.science/api/pith-number/Y32RW23IYIMF5PTGNGZAV7DCFE/graph.json","events_json":"https://pith.science/api/pith-number/Y32RW23IYIMF5PTGNGZAV7DCFE/events.json","paper":"https://pith.science/paper/Y32RW23I"},"agent_actions":{"view_html":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE","download_json":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE.json","view_paper":"https://pith.science/paper/Y32RW23I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.02137&json=true","fetch_graph":"https://pith.science/api/pith-number/Y32RW23IYIMF5PTGNGZAV7DCFE/graph.json","fetch_events":"https://pith.science/api/pith-number/Y32RW23IYIMF5PTGNGZAV7DCFE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE/action/storage_attestation","attest_author":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE/action/author_attestation","sign_citation":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE/action/citation_signature","submit_replication":"https://pith.science/pith/Y32RW23IYIMF5PTGNGZAV7DCFE/action/replication_record"}},"created_at":"2026-05-18T00:30:40.745243+00:00","updated_at":"2026-05-18T00:30:40.745243+00:00"}