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Fig. 7.
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Dependence of the specific intensities in two modes (top panel) and of the PD (bottom panel) on the angle to the normal for the same model atmosphere as in Fig. 6 for four photon energies, i.e., 1, 3, 10, and 50 keV, shown by black, red, magenta, and blue curves, respectively. Black solid and dashed curves coincide.
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