Is It Possible to Diagnose the Non-thermal Distributions from EIS Spectra?

Physics

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Scientific paper

It has been shown that two kinds of non-thermal electron distributions can origin in the solar corona. The first one is kappa-distribution with enhanced number of high energy particles. The second one, n-distribution, has enhanced number of particles in its maximum in comparison with the Maxwell distribution. A set of synthetic spectra for different values of parameters for both kinds of non-thermal distributions, electron density and the mean energy of distribution has been computed in the spectral range coresponding to the EIS A and EIS B detectors. The diagnostics of the basic parameters of plasma (electron density, the mean energy of distribution and the shape of the distribution function) is suggested. The suitability of lines which have been proposed for diagnostic is discussed.

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