{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:NR2G2M52PUCFQALWXU67YFHD4L","short_pith_number":"pith:NR2G2M52","schema_version":"1.0","canonical_sha256":"6c746d33ba7d04580176bd3dfc14e3e2d907ce9ba2af5ed1c730cd0f752ca8ea","source":{"kind":"arxiv","id":"1612.02856","version":1},"attestation_state":"computed","paper":{"title":"Hard X-Ray Emission from Partially Occulted Solar Flares: RHESSI Observations in Two Solar Cycles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Fatima Rubio da Costa, Frederic Effenberger, Lindsay Glesener, Mitsuo Oka, Pascal Saint Hilaire, S\\\"am Krucker, Vah\\'e Petrosian, Wei Liu","submitted_at":"2016-12-08T22:01:57Z","abstract_excerpt":"Flares close to the solar limb, where the footpoints are occulted, can reveal the spectrum and structure of the coronal loop-top source in X-rays. We aim at studying the properties of the corresponding energetic electrons near their acceleration site, without footpoint contamination. To this end, a statistical study of partially occulted flares observed with RHESSI is presented here, covering a large part of solar cycles 23 and 24. We perform a detailed spectra, imaging and light curve analysis for 116 flares and include contextual observations from SDO and STEREO when available, providing fur"},"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":"1612.02856","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-12-08T22:01:57Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"5cf642a62f7632e743b0aefb8f6a44bac6b7906fe3e2f29961dc6b30659ba06b","abstract_canon_sha256":"d56404a892fbf5929f710dea9ac512ce5043112d00a48ddbf86bbb0a48314b56"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:51:41.618295Z","signature_b64":"dOydoWEX+JlsIh/zEbmmIvhbktMgCdS9K1dv6J5LKq10xhg7+dSwgfn3hDjm6RpFjFxi0RFzx2s4sDWIGZ6lCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6c746d33ba7d04580176bd3dfc14e3e2d907ce9ba2af5ed1c730cd0f752ca8ea","last_reissued_at":"2026-05-18T00:51:41.617766Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:51:41.617766Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hard X-Ray Emission from Partially Occulted Solar Flares: RHESSI Observations in Two Solar Cycles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"astro-ph.SR","authors_text":"Fatima Rubio da Costa, Frederic Effenberger, Lindsay Glesener, Mitsuo Oka, Pascal Saint Hilaire, S\\\"am Krucker, Vah\\'e Petrosian, Wei Liu","submitted_at":"2016-12-08T22:01:57Z","abstract_excerpt":"Flares close to the solar limb, where the footpoints are occulted, can reveal the spectrum and structure of the coronal loop-top source in X-rays. We aim at studying the properties of the corresponding energetic electrons near their acceleration site, without footpoint contamination. To this end, a statistical study of partially occulted flares observed with RHESSI is presented here, covering a large part of solar cycles 23 and 24. We perform a detailed spectra, imaging and light curve analysis for 116 flares and include contextual observations from SDO and STEREO when available, providing fur"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.02856","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":"1612.02856","created_at":"2026-05-18T00:51:41.617835+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.02856v1","created_at":"2026-05-18T00:51:41.617835+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.02856","created_at":"2026-05-18T00:51:41.617835+00:00"},{"alias_kind":"pith_short_12","alias_value":"NR2G2M52PUCF","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"NR2G2M52PUCFQALW","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"NR2G2M52","created_at":"2026-05-18T12:30:36.002864+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/NR2G2M52PUCFQALWXU67YFHD4L","json":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L.json","graph_json":"https://pith.science/api/pith-number/NR2G2M52PUCFQALWXU67YFHD4L/graph.json","events_json":"https://pith.science/api/pith-number/NR2G2M52PUCFQALWXU67YFHD4L/events.json","paper":"https://pith.science/paper/NR2G2M52"},"agent_actions":{"view_html":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L","download_json":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L.json","view_paper":"https://pith.science/paper/NR2G2M52","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.02856&json=true","fetch_graph":"https://pith.science/api/pith-number/NR2G2M52PUCFQALWXU67YFHD4L/graph.json","fetch_events":"https://pith.science/api/pith-number/NR2G2M52PUCFQALWXU67YFHD4L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L/action/storage_attestation","attest_author":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L/action/author_attestation","sign_citation":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L/action/citation_signature","submit_replication":"https://pith.science/pith/NR2G2M52PUCFQALWXU67YFHD4L/action/replication_record"}},"created_at":"2026-05-18T00:51:41.617835+00:00","updated_at":"2026-05-18T00:51:41.617835+00:00"}