{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:XLUGSAJ5WFHVQIVGAA66RJ7NA5","short_pith_number":"pith:XLUGSAJ5","schema_version":"1.0","canonical_sha256":"bae869013db14f5822a6003de8a7ed074d99f18375186e0b995f07d06d186b2b","source":{"kind":"arxiv","id":"0808.3102","version":2},"attestation_state":"computed","paper":{"title":"Heavy Coronal Ions in the Heliosphere: I. Global Distribution of Charge-states of C, N, O, Mg, Si and S","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"M. Bzowski (1), M.E. Wachowicz (1), Moscow, Poland) ((2) Moscow State University, Russia), S. Grzedzielski (1), V. Izmodenov (2) ((1) Space Research Centre PAS, Warsaw","submitted_at":"2008-08-22T15:51:24Z","abstract_excerpt":"Aims: Investigate/Study de-charging of solar wind C, N, O, Mg, Si and S ions and assess fluxes of resulting ENA in the heliosphere. Methods: The model treats the heavy ions as test particles convected by (and in a particular case also diffusing through) a hydrodynamically calculated background plasma flow, from 1 AU to the termination shock (TS), to heliosheath (HS) and finally to heliospheric tail (HT). The ions undergo radiative and dielectronic recombinations, charge exchanges, photo- and electron impact ionizations with plasma particles, interstellar neutral atoms (calculated on a Monte-Ca"},"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":"0808.3102","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-08-22T15:51:24Z","cross_cats_sorted":[],"title_canon_sha256":"039b22e290768023aba241856920b948a1717b51ba6f97a81f3e4907a2d98e46","abstract_canon_sha256":"a0f0c2f6bb28c5109e5ad0c8c0648e6fbc821f0c6783c58146bf8f0a95103382"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:15:42.863621Z","signature_b64":"r0wWRGlJy2VF3hEJE/452nY4RyAkRzPnEUW9pJiZb3JRVw8AfR/au1j4dhdzxj9hRAUIRO+I8MyT17GU64VSBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bae869013db14f5822a6003de8a7ed074d99f18375186e0b995f07d06d186b2b","last_reissued_at":"2026-05-18T02:15:42.862974Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:15:42.862974Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Heavy Coronal Ions in the Heliosphere: I. Global Distribution of Charge-states of C, N, O, Mg, Si and S","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"M. Bzowski (1), M.E. Wachowicz (1), Moscow, Poland) ((2) Moscow State University, Russia), S. Grzedzielski (1), V. Izmodenov (2) ((1) Space Research Centre PAS, Warsaw","submitted_at":"2008-08-22T15:51:24Z","abstract_excerpt":"Aims: Investigate/Study de-charging of solar wind C, N, O, Mg, Si and S ions and assess fluxes of resulting ENA in the heliosphere. Methods: The model treats the heavy ions as test particles convected by (and in a particular case also diffusing through) a hydrodynamically calculated background plasma flow, from 1 AU to the termination shock (TS), to heliosheath (HS) and finally to heliospheric tail (HT). The ions undergo radiative and dielectronic recombinations, charge exchanges, photo- and electron impact ionizations with plasma particles, interstellar neutral atoms (calculated on a Monte-Ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0808.3102","kind":"arxiv","version":2},"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":"0808.3102","created_at":"2026-05-18T02:15:42.863072+00:00"},{"alias_kind":"arxiv_version","alias_value":"0808.3102v2","created_at":"2026-05-18T02:15:42.863072+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0808.3102","created_at":"2026-05-18T02:15:42.863072+00:00"},{"alias_kind":"pith_short_12","alias_value":"XLUGSAJ5WFHV","created_at":"2026-05-18T12:25:58.018023+00:00"},{"alias_kind":"pith_short_16","alias_value":"XLUGSAJ5WFHVQIVG","created_at":"2026-05-18T12:25:58.018023+00:00"},{"alias_kind":"pith_short_8","alias_value":"XLUGSAJ5","created_at":"2026-05-18T12:25:58.018023+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/XLUGSAJ5WFHVQIVGAA66RJ7NA5","json":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5.json","graph_json":"https://pith.science/api/pith-number/XLUGSAJ5WFHVQIVGAA66RJ7NA5/graph.json","events_json":"https://pith.science/api/pith-number/XLUGSAJ5WFHVQIVGAA66RJ7NA5/events.json","paper":"https://pith.science/paper/XLUGSAJ5"},"agent_actions":{"view_html":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5","download_json":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5.json","view_paper":"https://pith.science/paper/XLUGSAJ5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0808.3102&json=true","fetch_graph":"https://pith.science/api/pith-number/XLUGSAJ5WFHVQIVGAA66RJ7NA5/graph.json","fetch_events":"https://pith.science/api/pith-number/XLUGSAJ5WFHVQIVGAA66RJ7NA5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5/action/storage_attestation","attest_author":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5/action/author_attestation","sign_citation":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5/action/citation_signature","submit_replication":"https://pith.science/pith/XLUGSAJ5WFHVQIVGAA66RJ7NA5/action/replication_record"}},"created_at":"2026-05-18T02:15:42.863072+00:00","updated_at":"2026-05-18T02:15:42.863072+00:00"}