blue and cyan lines illustrate the times which MEGS-A and MEGS-B were exposed, respectively, while the horizontal purple line shows the time of the corresponding IRIS study. Lower-left panel: RHESSI lightcurves up to the maximum energy detected, with GOES start, peak, and end times overlaid. Right panel: A PROBA2/SWAP 174Å image taken near the peak of the flare. The white circle is 100$''$ wide centered on the location derived from AIA 131Å images, while the black contours mark out the 6–25keV emission observed by RHESSI. The fields of view of EIS, SOT, XRT, and IRIS are overplotted in green, yellow, red, and purple, respectively.[]{data-label="sff_plot"}](20140204_152500_M1_hsi100_megsab_eis_sot_xrt_iris.png){width="\textwidth"}

The *Ramaty High Energy Solar Spectroscopic Imager* {#ss:rhessi}
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RHESSI, launched on 5 February 2002[^8], observes the full disk of the Sun in X-rays and $\gamma$-rays. It orbits the Earth at an inclination angle of 38$^{\circ}$, at an altitude of $\approx$600 km, and as such suffers from eclipse passes and transits through the South Atlantic Anomaly. In order to determine whether or not RHESSI observed a given GOES flare event, the IDL routine was run between the start and end times of each flare. This searches the RHESSI flare catalog[^9] for the largest event detected in 