The radiation from Jupiter at this wavelength comes from ammonia gas in the stratosphere at a level of approximately 300 mbar with a brightness temperature of 130 K. The temperature sensitivity in this image is .15 K/arcsec rms. The R impact plume, shown near maximum brightness, has a 7.85 to 10.3 um color temperature of approximately 1500 K. For this display, the plume has been clipped at 7% peak intensity in order to show the features of the Jupiter disk. The prominent large bright areas to the right at the same Jupiter latitude are at the L and K impact sites. They are still a few degrees above their surroundings 1 1/2 days after the impacts.
MIRAC2 was built and is operated by the University of Arizona and the Smithsonian Astrophysical Observatory. It received support from the University of Arizona, Smithsonian Astrophysical Observatory, National Science Foundation, and National Aeronautics and Space Administration. It is operated and maintained by William F. Hoffmann (U/A), Giovanni G. Fazio (SAO), Joseph L. Hora (U. Hawaii), Lynne K. Deutsch (Boston Univ.), and Aditya Dayal (U/A). The camera utilizes a Rockwell HF-16 128 x 128 hybrid Si:As BIB array.
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