The bandwith was taken to be 120 kHz, integrationtime was about 1 sec smoothly averaged over 15 sec. This lightcurve was recorded with a 80 cm TV-satellite dish, mounted on the former 5 m Daedalus antenna dish. The small depression in the lightcurve right before the actual eclipse is thought to be due to a thunderstorm with strong rainfall. The solar eclipse as seen with our spectrometer Phoenix-2. The observed frequency range is from 700 MHz to 4000 MHz.
Low frequencies are on the top and high frequencies on the bottom of the plot.