Fig. 7.
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(a) Overview of the time period considered in this study (November 2020 to December 2022). Top: heliocentric distance of Solar Orbiter. Middle: monthly number of X-ray flares recorded by STIX. Bottom: monthly number of SEE events detected by EPD. (b): SEE events according to heliocentric distances of Solar Orbiter at the time of detection. The daily SEE rates for all distance bins are overplotted as red circles. The red error bars show the distance bins over which the rates were calculated.
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