{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:GGJTFCA232GI4HC7ZOV6M6QSUW","short_pith_number":"pith:GGJTFCA2","schema_version":"1.0","canonical_sha256":"319332881ade8c8e1c5fcbabe67a12a58786e08dbe7ef776fb2dcbee3c0cb2ad","source":{"kind":"arxiv","id":"1506.03548","version":1},"attestation_state":"computed","paper":{"title":"Atmosphere expansion and mass loss of close-orbit giant exoplanets heated by stellar XUV: I. Modeling of hydrodynamic escape of upper atmospheric material","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"H. Lammer, I. F. Shaikhislamov, K. G. Kislyakova, M. L. Khodachenko, N. V. Erkaev, Yu. L. Sasunov","submitted_at":"2015-06-11T05:47:32Z","abstract_excerpt":"In the present series of papers we propose a consistent description of the mass loss process. To study the effects of intrinsic magnetic field of a close-orbit giant exoplanet (so-called Hot Jupiter) on the atmospheric material escape and formation of planetary inner magnetosphere in a comprehensive way, we start with a hydrodynamic model of an upper atmosphere expansion presented in this paper. While considering a simple hydrogen atmosphere model, we focus on selfconsistent inclusion of the effects of radiative heating and ionization of the atmospheric gas with its consequent expansion in the"},"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":"1506.03548","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-06-11T05:47:32Z","cross_cats_sorted":[],"title_canon_sha256":"03711559e23fb76b9ae2fcc6f3d73b1c86920bbdd918899a8c0d1e89e3c86c9b","abstract_canon_sha256":"1901cc9399a740c7ace54a49a70c35cf1e0aba9ab927e434d27e7eea32d9a1ed"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:03.901659Z","signature_b64":"eOLrbtyDsxsaCgZfDOt5HDPW9Oy6/TgUAI0nTdK8YdrZqu3RFpL3EeE55iO7WK+dg14Z0m99BMLuEw+XippACw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"319332881ade8c8e1c5fcbabe67a12a58786e08dbe7ef776fb2dcbee3c0cb2ad","last_reissued_at":"2026-05-18T01:53:03.901136Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:03.901136Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Atmosphere expansion and mass loss of close-orbit giant exoplanets heated by stellar XUV: I. Modeling of hydrodynamic escape of upper atmospheric material","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"H. Lammer, I. F. Shaikhislamov, K. G. Kislyakova, M. L. Khodachenko, N. V. Erkaev, Yu. L. Sasunov","submitted_at":"2015-06-11T05:47:32Z","abstract_excerpt":"In the present series of papers we propose a consistent description of the mass loss process. To study the effects of intrinsic magnetic field of a close-orbit giant exoplanet (so-called Hot Jupiter) on the atmospheric material escape and formation of planetary inner magnetosphere in a comprehensive way, we start with a hydrodynamic model of an upper atmosphere expansion presented in this paper. While considering a simple hydrogen atmosphere model, we focus on selfconsistent inclusion of the effects of radiative heating and ionization of the atmospheric gas with its consequent expansion in the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.03548","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":"1506.03548","created_at":"2026-05-18T01:53:03.901207+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.03548v1","created_at":"2026-05-18T01:53:03.901207+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.03548","created_at":"2026-05-18T01:53:03.901207+00:00"},{"alias_kind":"pith_short_12","alias_value":"GGJTFCA232GI","created_at":"2026-05-18T12:29:22.688609+00:00"},{"alias_kind":"pith_short_16","alias_value":"GGJTFCA232GI4HC7","created_at":"2026-05-18T12:29:22.688609+00:00"},{"alias_kind":"pith_short_8","alias_value":"GGJTFCA2","created_at":"2026-05-18T12:29:22.688609+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/GGJTFCA232GI4HC7ZOV6M6QSUW","json":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW.json","graph_json":"https://pith.science/api/pith-number/GGJTFCA232GI4HC7ZOV6M6QSUW/graph.json","events_json":"https://pith.science/api/pith-number/GGJTFCA232GI4HC7ZOV6M6QSUW/events.json","paper":"https://pith.science/paper/GGJTFCA2"},"agent_actions":{"view_html":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW","download_json":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW.json","view_paper":"https://pith.science/paper/GGJTFCA2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.03548&json=true","fetch_graph":"https://pith.science/api/pith-number/GGJTFCA232GI4HC7ZOV6M6QSUW/graph.json","fetch_events":"https://pith.science/api/pith-number/GGJTFCA232GI4HC7ZOV6M6QSUW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW/action/storage_attestation","attest_author":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW/action/author_attestation","sign_citation":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW/action/citation_signature","submit_replication":"https://pith.science/pith/GGJTFCA232GI4HC7ZOV6M6QSUW/action/replication_record"}},"created_at":"2026-05-18T01:53:03.901207+00:00","updated_at":"2026-05-18T01:53:03.901207+00:00"}