{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:PTAGZK63N2R2FMYGJ5N5SVEKZM","short_pith_number":"pith:PTAGZK63","schema_version":"1.0","canonical_sha256":"7cc06cabdb6ea3a2b3064f5bd9548acb1c43d828b6e5fff45e525c94ce99010b","source":{"kind":"arxiv","id":"1505.00407","version":1},"attestation_state":"computed","paper":{"title":"Coronal sources and in situ properties of the solar winds sampled by ACE during 1999-2008","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bo Li, Chaozhou Mou, Fangran Jiao, Hui Fu, Lidong Xia, Xing Li, Zhenghua Huang","submitted_at":"2015-05-03T09:07:24Z","abstract_excerpt":"We identify the coronal sources of the solar winds sampled by the ACE spacecraft during 1999-2008, and examine the in situ solar wind properties as a function of wind sources. The standard two-step mapping technique is adopted to establish the photospheric footpoints of the magnetic flux tubes along which the ACE winds flow. The footpoints are then placed in the context of EIT 284~\\AA\\ images and photospheric magnetograms, allowing us to categorize the sources into four groups: coronal holes (CHs), active regions (ARs), the quiet Sun (QS), and \"Undefined\". This practice also enables us to esta"},"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":"1505.00407","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-05-03T09:07:24Z","cross_cats_sorted":[],"title_canon_sha256":"f4783780fb93609949463eba29c466f47108d50a90fadc267abcacbd8ead7b03","abstract_canon_sha256":"d4544e66d13141578b0b7aa182f357835f4eeb1eedd6ede2f7c670080f8819a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:17:10.250361Z","signature_b64":"/OCyGU/RklzevfSJ0RvycCiQu1RyqCJWsMXjbyYbqBg6nbXz+Cnphx0Jma9x5n+yESJmHzRe8cSVCknzjGM7Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7cc06cabdb6ea3a2b3064f5bd9548acb1c43d828b6e5fff45e525c94ce99010b","last_reissued_at":"2026-05-18T02:17:10.249699Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:17:10.249699Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Coronal sources and in situ properties of the solar winds sampled by ACE during 1999-2008","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bo Li, Chaozhou Mou, Fangran Jiao, Hui Fu, Lidong Xia, Xing Li, Zhenghua Huang","submitted_at":"2015-05-03T09:07:24Z","abstract_excerpt":"We identify the coronal sources of the solar winds sampled by the ACE spacecraft during 1999-2008, and examine the in situ solar wind properties as a function of wind sources. The standard two-step mapping technique is adopted to establish the photospheric footpoints of the magnetic flux tubes along which the ACE winds flow. The footpoints are then placed in the context of EIT 284~\\AA\\ images and photospheric magnetograms, allowing us to categorize the sources into four groups: coronal holes (CHs), active regions (ARs), the quiet Sun (QS), and \"Undefined\". This practice also enables us to esta"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.00407","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":"1505.00407","created_at":"2026-05-18T02:17:10.249823+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.00407v1","created_at":"2026-05-18T02:17:10.249823+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.00407","created_at":"2026-05-18T02:17:10.249823+00:00"},{"alias_kind":"pith_short_12","alias_value":"PTAGZK63N2R2","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_16","alias_value":"PTAGZK63N2R2FMYG","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_8","alias_value":"PTAGZK63","created_at":"2026-05-18T12:29:37.295048+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/PTAGZK63N2R2FMYGJ5N5SVEKZM","json":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM.json","graph_json":"https://pith.science/api/pith-number/PTAGZK63N2R2FMYGJ5N5SVEKZM/graph.json","events_json":"https://pith.science/api/pith-number/PTAGZK63N2R2FMYGJ5N5SVEKZM/events.json","paper":"https://pith.science/paper/PTAGZK63"},"agent_actions":{"view_html":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM","download_json":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM.json","view_paper":"https://pith.science/paper/PTAGZK63","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.00407&json=true","fetch_graph":"https://pith.science/api/pith-number/PTAGZK63N2R2FMYGJ5N5SVEKZM/graph.json","fetch_events":"https://pith.science/api/pith-number/PTAGZK63N2R2FMYGJ5N5SVEKZM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM/action/storage_attestation","attest_author":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM/action/author_attestation","sign_citation":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM/action/citation_signature","submit_replication":"https://pith.science/pith/PTAGZK63N2R2FMYGJ5N5SVEKZM/action/replication_record"}},"created_at":"2026-05-18T02:17:10.249823+00:00","updated_at":"2026-05-18T02:17:10.249823+00:00"}