THE CRYOGENIC LIMB ARRAY ETALON SPECTROMETER (CLAES) ON UARS - EXPERIMENT DESCRIPTION AND PERFORMANCE

Citation
Ae. Roche et al., THE CRYOGENIC LIMB ARRAY ETALON SPECTROMETER (CLAES) ON UARS - EXPERIMENT DESCRIPTION AND PERFORMANCE, JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 98(D6), 1993, pp. 10763-10775
Citations number
18
Categorie Soggetti
Metereology & Atmospheric Sciences
Volume
98
Issue
D6
Year of publication
1993
Pages
10763 - 10775
Database
ISI
SICI code
Abstract
The cryogenic limb array etalon spectrometer (CLAES) is one of 10 expe riments launched in September 1991 on the NASA Upper Atmosphere Resear ch Satellite (UARS). CLAES measures altitude profiles of temperature, pressure, O3, H2O, CH4, N2O, NO, NO2, N2O5, HNO3, ClONO2, HCl, CFC 11, CFC 12, and aerosol absorption coefficients. These data are obtained between 10 and 60 km with 2.5-km vertical resolution and 500-km horizo ntal grid size and between latitudes 80-degrees north and south. Since CLAES actually measures infrared spectral earthlimb emissions, it can operate continuously throughout the diurnal cycle. The on-orbit lifet ime as dictated by stored cryogens which cool optics and detectors is estimated to be 21 months. The experiment will perform the first globa l mapping of stratospheric ClONO2, CFC 11, CFC 12, and N2O5, and these data, along with the simultaneous measurement of temperature and the other constituents listed above, should contribute to a significant im provement in our understanding of stratospheric and mesospheric photoc hemistry, radiative structure, and dynamics. CLAES began viewing the a tmosphere in early October 1991, and the first several months of obser vations will be discussed. Examples of atmospheric spectral emission p rofiles for a number of constituents are presented as well as responsi vity and noise parameters. These data show the instrument performance to be excellent and close to prelaunch predictions. An overview of the experiment and instrumentation is presented, various scientific obser vational modes are described, and the algorithms and software used to retrieve atmospheric parameters from emission spectra are discussed.