2005/03/18 by F. Spineanu, M. Vlad, Spineanu, F. +1
Earth and Planetary Sciences · Physics and Astronomy · #Atmospheric and Oceanic Physics (physics.ao-ph) #FOS: Physical sciences #Ionosphere and magnetosphere dynamics #Plasma Physics (physics.plasm-ph) #Solar and Space Plasma Dynamics #Tropical and Extratropical Cyclones Research #physics.ao-ph #physics.plasm-ph
paper · pdf · doi:10.48550/arxiv.physics/0503155
Latex 37 pages. Corrected scales in figures
openalex publication_date 2005/03/18 · arxiv created 2005/03/31 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We present results of a numerical study of the differential equation governing the stationary states of the two-dimensional planetary atmosphere and magnetized plasma (within the Charney Hasegawa Mima model). The most strinking result is that the equation appears to be able to reproduce the main features of the flow structure of a typhoon.