Credits: Miteva, Klein, Samwel, Reid, Nindos and Kouloumvakos, Solar Physics (in prep.)
A stacked plot for each SEP event is prepared, whenever radio spectra are found. The radio spectra are ordered top-to-bottom as dm (ranging from 4500 to 800 MHz), m (from 800 to 20 MHz) and DH/km (0.02-14 MHz) wavelengths. These spectral plots are given together with the GOES SXR light curves (always on the top of each spectral graph). Since we use quick-look data as provided by the different observatories, the color table of the final compound plot is not uniform. Because the purpose of this catalog is a qualitative evaluation of the radio signatures we keep the original plots. In addition, the utilized plotting routine did not specify a uniform color code for the Wind/WAVES data.