Earth global mosaic observations with NIMS-Galileo

Abstract During the Earth-1 Galileo flyby (December 1990). the Near-Infrared Mapping Spectrometer (NIMS) experiment investigated the illuminated side of the Earth in the spectral range 0.7–5.2 μm. Mosaics of the entire terrestrial globe were recorded with a spatial resolution ranging from 100 to 500 km. From these spectra, information is retrieved upon the largescale temperature structure in the stratosphere and in the mesosphere (0–70 km altitude range) from the inversion of the CO 2 bands at 4.3 and 4.8 μm. These data also permit monitoring of the cloud temperatures, and derivation of the abundances of several minor atmospheric constituents (H 2 O, CO, N 2 O. CH 4 and O 3 ). These observations constitute a continuation of the study of the atmospheres of the three planets (i.e. Venus, the Earth and Jupiter) targeted by the Galileo spacecraft during its mission. Observing these atmospheres with the NIMS instrument in the near-infrared will provide a unique data set, useful for comparative planetary studies.