2008/05/31 by N. S. Dzhalilov, V. D. Kuznetsov, J. Staude
Physics and Astronomy · #Dust and Plasma Wave Phenomena #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809882
published as Astron. Astrophys. 489, 769-772, 2008 · 5 pages, length reduced to that of a Research Note, A&A (in press)
openalex publication_date 2008/08/08 · arxiv created 2008/09/02 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01
Aims. We study wave instability in an collisionless, rarefied hot plasma (e.g. solar wind or corona). We consider the anisotropy produced by the magnetic field, when the thermal gas pressures across and along the field become unequal.