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Theory of heating of hot magnetized plasma by Alfven waves. Application for solar corona
T. M. Mishonov, M. V. Stoev, Y. G. Maneva
The heating of magnetized plasma by propagation of Alfven waves is calculated as a function of the magnetic field spectral density. The results can be applied to evaluate the heati…
On the origin of solar wind. Alfven waves induced jump of coronal temperature
T. M. Mishonov, M. V. Stoev, Y. G. Maneva
Absorbtion of Alfven waves is considered to be the main mechanism of heating in the solar corona. It is concluded that the sharp increase of the plasma temperature by two orders of…
Burgulence and Alfven waves heating mechanism of solar corona
T. M. Mishonov, Y. G. Maneva
Heating of magnetized turbulent plasma is calculated in the framework of Burgers turbulence [A.M. Polyakov, Phys. Rev. E. 52, 6183 (1995)]. Explicit formula for the energy flux of…
On the theory of MHD waves in a shear flow of a magnetized turbulent plasma
T. M. Mishonov, Y. G. Maneva, Z. D. Dimitrov +1
The set of equations for magnetohydrodynamic (MHD) waves in a shear flow is consecutively derived. The proposed scenario involves the presence of a self-sustained turbulence and ma…