{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:ZRUMQ7MDXHK3NFOXUJTO6OOZTT","short_pith_number":"pith:ZRUMQ7MD","schema_version":"1.0","canonical_sha256":"cc68c87d83b9d5b695d7a266ef39d99ce0c085e58ce092f438f454ca7832cd7f","source":{"kind":"arxiv","id":"1112.2967","version":1},"attestation_state":"computed","paper":{"title":"Solar parameters for modeling interplanetary background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D.J. McComas, E. Quemerais, J.M. Sokol, K. Fujiki, M. Bzowski, M. Tokumaru, P. Bochsler, R. Lallement, S. Ferron","submitted_at":"2011-12-13T17:18:30Z","abstract_excerpt":"The goal of the Fully Online Datacenter of Ultraviolet Emissions (FONDUE) Working Team of the International Space Science Institute in Bern, Switzerland, was to establish a common calibration of various UV and EUV heliospheric observations, both spectroscopic and photometric. Realization of this goal required an up-to-date model of spatial distribution of neutral interstellar hydrogen in the heliosphere, and to that end, a credible model of the radiation pressure and ionization processes was needed. This chapter describes the solar factors shaping the distribution of neutral interstellar H in "},"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":"1112.2967","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-12-13T17:18:30Z","cross_cats_sorted":[],"title_canon_sha256":"c5a2d103e9ca6201e8cef0196444e154ad1bccc0c9b781f2e2d160b0be97437e","abstract_canon_sha256":"85ad3336fc4ca58ce3885e428d2dffc28b4d5a8584414c279f2985459631bc86"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:10.741897Z","signature_b64":"jEokTHsgIx/Oh4mmXBLQrlkqSwo4+NzzJ6pcO/h5S1Rmh7VchxYCcA+Xz1ECsU1qOJV4+Bxh0r3cT9SgEEUxDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc68c87d83b9d5b695d7a266ef39d99ce0c085e58ce092f438f454ca7832cd7f","last_reissued_at":"2026-05-18T01:59:10.741216Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:10.741216Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar parameters for modeling interplanetary background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D.J. McComas, E. Quemerais, J.M. Sokol, K. Fujiki, M. Bzowski, M. Tokumaru, P. Bochsler, R. Lallement, S. Ferron","submitted_at":"2011-12-13T17:18:30Z","abstract_excerpt":"The goal of the Fully Online Datacenter of Ultraviolet Emissions (FONDUE) Working Team of the International Space Science Institute in Bern, Switzerland, was to establish a common calibration of various UV and EUV heliospheric observations, both spectroscopic and photometric. Realization of this goal required an up-to-date model of spatial distribution of neutral interstellar hydrogen in the heliosphere, and to that end, a credible model of the radiation pressure and ionization processes was needed. This chapter describes the solar factors shaping the distribution of neutral interstellar H in "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.2967","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":"1112.2967","created_at":"2026-05-18T01:59:10.741327+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.2967v1","created_at":"2026-05-18T01:59:10.741327+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.2967","created_at":"2026-05-18T01:59:10.741327+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZRUMQ7MDXHK3","created_at":"2026-05-18T12:26:50.516681+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZRUMQ7MDXHK3NFOX","created_at":"2026-05-18T12:26:50.516681+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZRUMQ7MD","created_at":"2026-05-18T12:26:50.516681+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/ZRUMQ7MDXHK3NFOXUJTO6OOZTT","json":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT.json","graph_json":"https://pith.science/api/pith-number/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/graph.json","events_json":"https://pith.science/api/pith-number/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/events.json","paper":"https://pith.science/paper/ZRUMQ7MD"},"agent_actions":{"view_html":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT","download_json":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT.json","view_paper":"https://pith.science/paper/ZRUMQ7MD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.2967&json=true","fetch_graph":"https://pith.science/api/pith-number/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/graph.json","fetch_events":"https://pith.science/api/pith-number/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/action/storage_attestation","attest_author":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/action/author_attestation","sign_citation":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/action/citation_signature","submit_replication":"https://pith.science/pith/ZRUMQ7MDXHK3NFOXUJTO6OOZTT/action/replication_record"}},"created_at":"2026-05-18T01:59:10.741327+00:00","updated_at":"2026-05-18T01:59:10.741327+00:00"}