Measurement of energies of MHD waves generated by a microflare by SOLAR-B
T. Yokoyama
The dissipation of MHD waves is suggested as a possible mechanism of
the coronal heating. The measurement of the wave energy and its dissipation
rate is one of the most important subjects that have to be studied during
the SOLAR-B project. In this paper, we will discuss how to measure by SOLAR-B
the wave energy generated by a flare or a microflare.
By using the three-dimensional simulations of propagation of linear MHD
waves, the predicted profiles of SOLAR-B/EIS data as a function of
the wavelength, time, and space are presented.
Correspondence
T. Yokoyama (yokoyama.t@eps.s.u-tokyo.ac.jp), University of Tokyo
Preference of Presentation
poster