Relative drifts and temperature anisotropies of protons andαparticles in the expanding solar wind: 2.5D hybrid simulations

2014/10/10 by Y. G. Maneva, L. Ofman, A. Viñas · 1 citation
Physics and Astronomy · #Anisotropy #Dust and Plasma Wave Phenomena #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics #Solar energetic particles #Solar flare #Solar physics #Solar wind #Turbulence #physics.space-ph

paper · pdf · doi:10.1051/0004-6361/201424401

published as A&A 578, A85 (2015) · 11 pages, 13 figures, submitted to A&A

arxiv created 2014/10/10 · openalex publication_date 2015/05/09 · arxiv updated 2015/06/11 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. We perform 2.5D hybrid simulations to investigate the origin and evolution of relative drift speeds between protons and α particles in the collisionless turbulent low- solar wind plasma.

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