Abstract:In this paper, (pure, slow, and fast) Alfvèn waves for the accepted conditions in Northernhemisphere at E-region of ionospheric plasma were calculated with low latitudes by using Eq. (20,(25)(26) and the real geometry of Earth's magnetic field, at hours 12.00 LT for the 1990 year which sunspot is maximum. One of the most important results of this study is to show analytically that the "MHD modes= (pure, slow and fast) Alfvèn waves" depend not only on the angle between the wave propagation vector (k) and the ma… Show more
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