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Fig. 4.

Fig. 4. Refer to the following caption and surrounding text.

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DAXSS spectra corresponding to the lowest and highest count rates in the DAXSS light curve along with arbitrarily scaled SaXS models of the various types of coronal regions. This demonstrates the steeper slope of the solar spectra compared with the spectrum of all types of coronal region which indicates an over-contribution of low-signal EM bins (see text in Sect. 3.2).

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