{"paper":{"title":"The statistical properties of solar wind temperature parameters near 1 AU","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"Bennett A. Maruca, Chadi S. Salem, Justin C. Kasper, Kristopher G. Klein, Lynn B. Wilson III, Marc P. Pulupa, Michael L. Stevens, Stuart D. Bale, Trevor A. Bowen","submitted_at":"2018-02-23T15:15:26Z","abstract_excerpt":"We present a long-duration ($\\sim$10 years) statistical analysis of the temperatures, plasma betas, and temperature ratios for the electron, proton, and alpha-particle populations observed by the \\emph{Wind} spacecraft near 1 AU. The mean(median) scalar temperatures are $T{\\scriptstyle_{e, tot}}$ $=$ 12.2(11.9) eV, $T{\\scriptstyle_{p, tot}}$ $=$ 12.7(8.6) eV, and $T{\\scriptstyle_{\\alpha, tot}}$ $=$ 23.9(10.8) eV. The mean(median) total plasma betas are $\\beta{\\scriptstyle_{e, tot}}$ $=$ 2.31(1.09), $\\beta{\\scriptstyle_{p, tot}}$ $=$ 1.79(1.05), and $\\beta{\\scriptstyle_{\\alpha, tot}}$ $=$ 0.17("},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.08585","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"}