{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:ICACV5UYEI7OFSVPNTKO4D6BI7","short_pith_number":"pith:ICACV5UY","schema_version":"1.0","canonical_sha256":"40802af698223ee2caaf6cd4ee0fc147d866a7f4e6cf4177874f2a0a0520f3a0","source":{"kind":"arxiv","id":"1508.06003","version":1},"attestation_state":"computed","paper":{"title":"Hard X-Ray Imaging of Individual Spectral Components in Solar Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR","physics.plasm-ph","physics.space-ph"],"primary_cat":"astro-ph.IM","authors_text":"Albert Y. Shih, Amir Caspi, James M. McTiernan, S\\\"am Krucker","submitted_at":"2015-08-25T01:21:39Z","abstract_excerpt":"We present a new analytical technique, combining Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) high-resolution imaging and spectroscopic observations, to visualize solar flare emission as a function of spectral component (e.g., isothermal temperature) rather than energy. This computationally inexpensive technique is applicable to all spatially-invariant spectral forms and is useful for visualizing spectroscopically-determined individual sources and placing them in context, e.g., comparing multiple isothermal sources with nonthermal emission locations. For example, while extreme"},"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":"1508.06003","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-08-25T01:21:39Z","cross_cats_sorted":["astro-ph.HE","astro-ph.SR","physics.plasm-ph","physics.space-ph"],"title_canon_sha256":"bc30db1bbf6c51b3ff1b000fac43b83fa9b2056bafc9b7d3cace004b361e5e10","abstract_canon_sha256":"e5eb1fd3227c6ca85a1bbbdfcbea446cca71b05a18e9cde334e5031f4e386b98"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:33:15.195075Z","signature_b64":"LRAI3m5HtjWbdu3bFgvr4+KJBMcYX4xJsGOvqtn+j1CTycjwuIk1KAge9qENHLLsiVmNBot1ON1FP7yy2rfHDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40802af698223ee2caaf6cd4ee0fc147d866a7f4e6cf4177874f2a0a0520f3a0","last_reissued_at":"2026-05-18T01:33:15.194406Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:33:15.194406Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hard X-Ray Imaging of Individual Spectral Components in Solar Flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR","physics.plasm-ph","physics.space-ph"],"primary_cat":"astro-ph.IM","authors_text":"Albert Y. Shih, Amir Caspi, James M. McTiernan, S\\\"am Krucker","submitted_at":"2015-08-25T01:21:39Z","abstract_excerpt":"We present a new analytical technique, combining Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) high-resolution imaging and spectroscopic observations, to visualize solar flare emission as a function of spectral component (e.g., isothermal temperature) rather than energy. This computationally inexpensive technique is applicable to all spatially-invariant spectral forms and is useful for visualizing spectroscopically-determined individual sources and placing them in context, e.g., comparing multiple isothermal sources with nonthermal emission locations. For example, while extreme"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.06003","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":"1508.06003","created_at":"2026-05-18T01:33:15.194526+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.06003v1","created_at":"2026-05-18T01:33:15.194526+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.06003","created_at":"2026-05-18T01:33:15.194526+00:00"},{"alias_kind":"pith_short_12","alias_value":"ICACV5UYEI7O","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_16","alias_value":"ICACV5UYEI7OFSVP","created_at":"2026-05-18T12:29:25.134429+00:00"},{"alias_kind":"pith_short_8","alias_value":"ICACV5UY","created_at":"2026-05-18T12:29:25.134429+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/ICACV5UYEI7OFSVPNTKO4D6BI7","json":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7.json","graph_json":"https://pith.science/api/pith-number/ICACV5UYEI7OFSVPNTKO4D6BI7/graph.json","events_json":"https://pith.science/api/pith-number/ICACV5UYEI7OFSVPNTKO4D6BI7/events.json","paper":"https://pith.science/paper/ICACV5UY"},"agent_actions":{"view_html":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7","download_json":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7.json","view_paper":"https://pith.science/paper/ICACV5UY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.06003&json=true","fetch_graph":"https://pith.science/api/pith-number/ICACV5UYEI7OFSVPNTKO4D6BI7/graph.json","fetch_events":"https://pith.science/api/pith-number/ICACV5UYEI7OFSVPNTKO4D6BI7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7/action/storage_attestation","attest_author":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7/action/author_attestation","sign_citation":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7/action/citation_signature","submit_replication":"https://pith.science/pith/ICACV5UYEI7OFSVPNTKO4D6BI7/action/replication_record"}},"created_at":"2026-05-18T01:33:15.194526+00:00","updated_at":"2026-05-18T01:33:15.194526+00:00"}