{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:36BZEZAJZ5JAD2LUQ56ATAZUNZ","short_pith_number":"pith:36BZEZAJ","schema_version":"1.0","canonical_sha256":"df83926409cf5201e974877c0983346e74e8a0a3abe4502aee163dd32a99594f","source":{"kind":"arxiv","id":"1709.01605","version":1},"attestation_state":"computed","paper":{"title":"Interfacing MHD Single Fluid and Kinetic Exospheric Solar Wind Models and Comparing Their Energetics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jens Pomoell, Rony Keppens, Sofia-Paraskevi Moschou, Viviane Pierrard","submitted_at":"2017-09-05T21:57:12Z","abstract_excerpt":"An exospheric kinetic solar wind model is interfaced with an observation-driven single fluid magnetohydrodynamic (MHD) model. Initially, a photospheric magnetogram serves as observational input in the fluid approach to extrapolate the heliospheric magnetic field. Then semi-empirical coronal models are used for estimating the plasma characteristics up to a heliocentric distance of 0.1AU. From there on a full MHD model which computes the three-dimensional time-dependent evolution of the solar wind macroscopic variables up to the orbit of the Earth is used. After interfacing the density and veloc"},"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":"1709.01605","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-09-05T21:57:12Z","cross_cats_sorted":[],"title_canon_sha256":"3a6482abcec95b67c33d73c7bdd51fd6f8a9ed43ffb9c0f4fb647cefe7905c53","abstract_canon_sha256":"5ba54219e3a0ac1b433ebbb8066f2c0cf08bed56c243519f1e018584bdde1fcf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:33:48.262882Z","signature_b64":"ir68orvx4drpA9bSLSRZUK2c8sXf48q/aLGaV/IwkmEOWH3lMMsQiUo3BiYFINAGfnzYA9q/oKbIuT3d0MQ4CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"df83926409cf5201e974877c0983346e74e8a0a3abe4502aee163dd32a99594f","last_reissued_at":"2026-05-18T00:33:48.262198Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:33:48.262198Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interfacing MHD Single Fluid and Kinetic Exospheric Solar Wind Models and Comparing Their Energetics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jens Pomoell, Rony Keppens, Sofia-Paraskevi Moschou, Viviane Pierrard","submitted_at":"2017-09-05T21:57:12Z","abstract_excerpt":"An exospheric kinetic solar wind model is interfaced with an observation-driven single fluid magnetohydrodynamic (MHD) model. Initially, a photospheric magnetogram serves as observational input in the fluid approach to extrapolate the heliospheric magnetic field. Then semi-empirical coronal models are used for estimating the plasma characteristics up to a heliocentric distance of 0.1AU. From there on a full MHD model which computes the three-dimensional time-dependent evolution of the solar wind macroscopic variables up to the orbit of the Earth is used. After interfacing the density and veloc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.01605","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":"1709.01605","created_at":"2026-05-18T00:33:48.262295+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.01605v1","created_at":"2026-05-18T00:33:48.262295+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.01605","created_at":"2026-05-18T00:33:48.262295+00:00"},{"alias_kind":"pith_short_12","alias_value":"36BZEZAJZ5JA","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"36BZEZAJZ5JAD2LU","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"36BZEZAJ","created_at":"2026-05-18T12:30:58.224056+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/36BZEZAJZ5JAD2LUQ56ATAZUNZ","json":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ.json","graph_json":"https://pith.science/api/pith-number/36BZEZAJZ5JAD2LUQ56ATAZUNZ/graph.json","events_json":"https://pith.science/api/pith-number/36BZEZAJZ5JAD2LUQ56ATAZUNZ/events.json","paper":"https://pith.science/paper/36BZEZAJ"},"agent_actions":{"view_html":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ","download_json":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ.json","view_paper":"https://pith.science/paper/36BZEZAJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.01605&json=true","fetch_graph":"https://pith.science/api/pith-number/36BZEZAJZ5JAD2LUQ56ATAZUNZ/graph.json","fetch_events":"https://pith.science/api/pith-number/36BZEZAJZ5JAD2LUQ56ATAZUNZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ/action/storage_attestation","attest_author":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ/action/author_attestation","sign_citation":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ/action/citation_signature","submit_replication":"https://pith.science/pith/36BZEZAJZ5JAD2LUQ56ATAZUNZ/action/replication_record"}},"created_at":"2026-05-18T00:33:48.262295+00:00","updated_at":"2026-05-18T00:33:48.262295+00:00"}