{"paper":{"title":"Implications of solar wind measurements for solar models and composition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","nucl-ex"],"primary_cat":"astro-ph.SR","authors_text":"Aaron C. Vincent (IPPP, Aldo Serenelli (ICE/CSIC-IEEC), Carlos Pena-Garay (IFIC/CSIC & Canfranc), Durham), Francesco L. Villante (Univ. L'Aquila & LNGS), Martin Asplund (ANU), Nicolas Grevesse (Univ. Leige), Pat Scott (Imperial Coll.), Sarbani Basu (Yale Univ.)","submitted_at":"2016-04-18T20:00:06Z","abstract_excerpt":"We critically examine recent claims of a high solar metallicity by von Steiger \\& Zurbuchen (2016) based on \\textit{in situ} measurements of the solar wind, rather than the standard spectroscopically-inferred abundances (Asplund et al. 2009). We test the claim by Vagnozzi et al. (2016) that a composition based on the solar wind enables one to construct a standard solar model in agreement with helioseismological observations and thus solve the decades-old solar modelling problem. We show that, although some helioseismological observables are improved compared to models computed with spectroscop"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.05318","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"}