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Earth, Planets and Space
Fig. 6 | Earth, Planets and Space

Fig. 6

From: Role of hard X-ray emission in ionospheric D-layer disturbances during solar flares

Fig. 6

Time profiles for three flares, M5.8 (April 3, 2017), X2.2 (September 6, 2017) and X8.2 (September 10, 2017) from left to right. For each event, the top and middle panels display RHESSI profiles (respectively, in the energy band 6 to 40 kev and 40 to 100 keV) and the bottom panel displays the two energy bands of GOES. The black arrows indicate the peak time of SXR and the blue arrows the peak time of the 40 keV emission

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