{"paper":{"title":"Temperature anisotropy instabilities of solar wind electrons with regularized Kappa-halos resolved with ALPS","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"physics.plasm-ph","authors_text":"(2) Centre for mathematical Plasma-Astrophysics, 3001 Leuven, (3) Mullard Space Science Laboratory, (4) Department of Planetary Science, Belgium, D-44780 Bochum, Daniel Verscharen (3), Dorking RH5 6NT, Dustin L. Schr\\\"oder (1), Germany, Horst Fichtner (1), Kristopher G. Klein (4) ((1) Institut f\\\"ur Theoretische Physik, KU Leuven, Lehrstuhl IV: Plasma-Astroteilchenphysik, Marian Lazar (2), Ruhr-Universit\\\"at Bochum, Tucson, UK, University College London, University of Arizona, USA)","submitted_at":"2025-04-22T14:50:39Z","abstract_excerpt":"Space plasmas in various astrophysical setups can often be both very hot and dilute, making them highly susceptible to waves and fluctuations, which are generally self-generated and maintained by kinetic instabilities. In this sense, we have in-situ observational evidence from the solar wind and planetary environments, which reveal not only wave fluctuations at kinetic scales of electrons and protons, but also non-equilibrium distributions of particle velocities. This paper reports on the progress made in achieving a consistent modeling of the instabilities generated by temperature anisotropy,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.15955","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2504.15955/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}