Wed Jul 20 16:52:32 1994
Because of mail difficulties, our reports have not been getting out. With the Rochester 256 x 256 InSb camera at WIRO, the Wyoming Infrared Observatory, we have been observing Jupiter at wavelengths from 1.25 to 4.5 microns with a 2.5% CVF whenever feasible. To date, only the B impact was not clouded out. In that case we obtained at 2.2 microns a time series of 940 observations of part of Jupiter, the rings, and Amalthea, for about 1.5 hours.
Continuing spectral images of the sites of the various impacts have been obtained at a series of wavelengths from 1.25 to 4.5 microns at 2.5% resolution whenever Jupiter is available.