2011/04/01 by Francisco Caruso, Caruso, Francisco, V. Oguri +1
Physics and Astronomy · #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #Dust and Plasma Wave Phenomena #FOS: Physical sciences #Ionosphere and magnetosphere dynamics #Plasma Physics (physics.plasm-ph) #Solar and Space Plasma Dynamics
paper · pdf · doi:10.48550/arxiv.1104.0229
openalex publication_date 2011/04/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
Magnetic fluctuations in a non-magnetized gaseous plasma is revisited and calculated without approximations, based on the fluctuation-dissipation theorem. It is argued that the present results are qualitative and quantitative different form previous one based on the same theorem. In particular, it is shown that it is not correct that the spectral intensity does not vary sensitively with kcut. Also the simultaneous dependence of this intensity on the plasma and on the collisional frequencies are discussed.