{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:CRAAYIKQE2SRMJZ5HQACMJMMBU","short_pith_number":"pith:CRAAYIKQ","schema_version":"1.0","canonical_sha256":"14400c215026a516273d3c0026258c0d2ade10be3459bc556420a37d45fa7fd1","source":{"kind":"arxiv","id":"2206.00964","version":3},"attestation_state":"computed","paper":{"title":"The solar disk at high energies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Manuel Masip, Miguel Guti\\'errez, Sergio Mu\\~noz","submitted_at":"2022-06-02T09:58:03Z","abstract_excerpt":"High energy cosmic rays \"illuminate\" the Sun and produce an image that could be observed in up to five different channels: a cosmic ray shadow (whose energy dependence has been studied by HAWC); a gamma ray flux (observed at $E\\le 200$ GeV by Fermi-LAT); a muon shadow (detected by ANTARES and IceCube); a neutron flux (undetected, as there are no hadronic calorimeters in space); and a flux of high energy neutrinos. Since these signals are correlated, the ones already observed can be used to reduce the uncertainty in the still undetected ones. Here we define a simple set up that uses the Fermi-L"},"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":"2206.00964","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-06-02T09:58:03Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"696bac67c6965f02c45b561fec446d811bcaf07671a9da128992830e14a99d30","abstract_canon_sha256":"a3164e01c7fc7142aa778288513de1793a47453bb511d8c78da744138384c416"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:22:58.431138Z","signature_b64":"KT/oxey1seN7hF7TaY9znQteBoEe21KtD/hu3v6r0VN5bEc2InWkNLAtf4XJbRdSjzHlZBndVC+6cSshiJNdDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14400c215026a516273d3c0026258c0d2ade10be3459bc556420a37d45fa7fd1","last_reissued_at":"2026-07-05T06:22:58.430727Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:22:58.430727Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The solar disk at high energies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Manuel Masip, Miguel Guti\\'errez, Sergio Mu\\~noz","submitted_at":"2022-06-02T09:58:03Z","abstract_excerpt":"High energy cosmic rays \"illuminate\" the Sun and produce an image that could be observed in up to five different channels: a cosmic ray shadow (whose energy dependence has been studied by HAWC); a gamma ray flux (observed at $E\\le 200$ GeV by Fermi-LAT); a muon shadow (detected by ANTARES and IceCube); a neutron flux (undetected, as there are no hadronic calorimeters in space); and a flux of high energy neutrinos. Since these signals are correlated, the ones already observed can be used to reduce the uncertainty in the still undetected ones. Here we define a simple set up that uses the Fermi-L"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.00964","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2206.00964/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2206.00964","created_at":"2026-07-05T06:22:58.430785+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.00964v3","created_at":"2026-07-05T06:22:58.430785+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.00964","created_at":"2026-07-05T06:22:58.430785+00:00"},{"alias_kind":"pith_short_12","alias_value":"CRAAYIKQE2SR","created_at":"2026-07-05T06:22:58.430785+00:00"},{"alias_kind":"pith_short_16","alias_value":"CRAAYIKQE2SRMJZ5","created_at":"2026-07-05T06:22:58.430785+00:00"},{"alias_kind":"pith_short_8","alias_value":"CRAAYIKQ","created_at":"2026-07-05T06:22:58.430785+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.08726","citing_title":"Angular Distribution of Gamma Rays Produced in Proton-Proton Collisions","ref_index":24,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU","json":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU.json","graph_json":"https://pith.science/api/pith-number/CRAAYIKQE2SRMJZ5HQACMJMMBU/graph.json","events_json":"https://pith.science/api/pith-number/CRAAYIKQE2SRMJZ5HQACMJMMBU/events.json","paper":"https://pith.science/paper/CRAAYIKQ"},"agent_actions":{"view_html":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU","download_json":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU.json","view_paper":"https://pith.science/paper/CRAAYIKQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.00964&json=true","fetch_graph":"https://pith.science/api/pith-number/CRAAYIKQE2SRMJZ5HQACMJMMBU/graph.json","fetch_events":"https://pith.science/api/pith-number/CRAAYIKQE2SRMJZ5HQACMJMMBU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU/action/storage_attestation","attest_author":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU/action/author_attestation","sign_citation":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU/action/citation_signature","submit_replication":"https://pith.science/pith/CRAAYIKQE2SRMJZ5HQACMJMMBU/action/replication_record"}},"created_at":"2026-07-05T06:22:58.430785+00:00","updated_at":"2026-07-05T06:22:58.430785+00:00"}