Fig. 10

LRTTM EL-I type instantaneous energy deposits (left) and HXR spectra (right) for the VAL C atmosphere at t = 0.3 s. The solid (MFF) and dotted (MSU) blue, green, red, yellow, and orange lines correspond to V m-1 and var(EL) = 0.1,0.5,1,2,5 V m-1, respectively, and energy flux ℱ0/2 = 2.5 × 109 erg cm-2 s-1. The dashed and solid grey lines correspond to the CTTM with ℱ0/2 = 2.5 × 109 and 5 × 1010 erg cm-2 s-1, respectively. The dotted straight vertical line indicates the bottom boundary of the magnetic mirror, the grey area the secondary re-acceleration region. The HXR spectra are integrated over one half of the loop.
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