{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:M5WOW2TX2PKWTHCAJMKHCNLPMH","short_pith_number":"pith:M5WOW2TX","schema_version":"1.0","canonical_sha256":"676ceb6a77d3d5699c404b1471356f61ee096d06d721b2df219093f0e4fc8d39","source":{"kind":"arxiv","id":"1705.02053","version":1},"attestation_state":"computed","paper":{"title":"Magnetic Flux Emergence and Decay Rates for Preceder and Follower Sunspots Observed with HMI","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. A. Norton, E. H. Jones, J. E. Leake, M. G. Linton","submitted_at":"2017-05-05T00:51:39Z","abstract_excerpt":"We quantify the emergence and decay rates of preceder (p) and follower (f) sunspots within ten active regions from 2010-2014 using Space-weather Helioseismic Magnetic Imager Active Region Patch data. The sunspots are small- to mid-sized regions and contain a signed flux within a single polarity sunspot of $(1.1-6.5)\\times 10^{21}$ Mx. The net unsigned flux within the regions, including plage, ranges from $(5.1-20)\\times 10^{21}$ Mx. Rates are calculated with and without intensity contours to differentiate between sunspot formation and flux emergence. Signed flux emergence rates, calculated wit"},"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":"1705.02053","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-05-05T00:51:39Z","cross_cats_sorted":[],"title_canon_sha256":"be0c0eb563407a74f8787812b9de841b0b06cfff4edb63cf816294a4c49ffb94","abstract_canon_sha256":"fade08dda2378fefec224781fcbafc8d75ccc13beb1b1b11d87f7101526556c6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:41:59.072120Z","signature_b64":"xY9IOyC9q6hihSa/tCIvnr2L3M6T/QBeh4s/r0w8/Ir/mgkfSF4Zl5azFdDAAikRsysTBR+rcc0DVoWHgKk5DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"676ceb6a77d3d5699c404b1471356f61ee096d06d721b2df219093f0e4fc8d39","last_reissued_at":"2026-05-18T00:41:59.071615Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:41:59.071615Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Magnetic Flux Emergence and Decay Rates for Preceder and Follower Sunspots Observed with HMI","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. A. Norton, E. H. Jones, J. E. Leake, M. G. Linton","submitted_at":"2017-05-05T00:51:39Z","abstract_excerpt":"We quantify the emergence and decay rates of preceder (p) and follower (f) sunspots within ten active regions from 2010-2014 using Space-weather Helioseismic Magnetic Imager Active Region Patch data. The sunspots are small- to mid-sized regions and contain a signed flux within a single polarity sunspot of $(1.1-6.5)\\times 10^{21}$ Mx. The net unsigned flux within the regions, including plage, ranges from $(5.1-20)\\times 10^{21}$ Mx. Rates are calculated with and without intensity contours to differentiate between sunspot formation and flux emergence. Signed flux emergence rates, calculated wit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.02053","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":"1705.02053","created_at":"2026-05-18T00:41:59.071688+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.02053v1","created_at":"2026-05-18T00:41:59.071688+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.02053","created_at":"2026-05-18T00:41:59.071688+00:00"},{"alias_kind":"pith_short_12","alias_value":"M5WOW2TX2PKW","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"M5WOW2TX2PKWTHCA","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"M5WOW2TX","created_at":"2026-05-18T12:31:28.150371+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/M5WOW2TX2PKWTHCAJMKHCNLPMH","json":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH.json","graph_json":"https://pith.science/api/pith-number/M5WOW2TX2PKWTHCAJMKHCNLPMH/graph.json","events_json":"https://pith.science/api/pith-number/M5WOW2TX2PKWTHCAJMKHCNLPMH/events.json","paper":"https://pith.science/paper/M5WOW2TX"},"agent_actions":{"view_html":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH","download_json":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH.json","view_paper":"https://pith.science/paper/M5WOW2TX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.02053&json=true","fetch_graph":"https://pith.science/api/pith-number/M5WOW2TX2PKWTHCAJMKHCNLPMH/graph.json","fetch_events":"https://pith.science/api/pith-number/M5WOW2TX2PKWTHCAJMKHCNLPMH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH/action/storage_attestation","attest_author":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH/action/author_attestation","sign_citation":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH/action/citation_signature","submit_replication":"https://pith.science/pith/M5WOW2TX2PKWTHCAJMKHCNLPMH/action/replication_record"}},"created_at":"2026-05-18T00:41:59.071688+00:00","updated_at":"2026-05-18T00:41:59.071688+00:00"}