Serabyn, E. and Weisstein, E. W. and Lis, D. C. (1995) FTS atmospheric transmission measurements and observations of planetary atmospheres. In: The Physics and Chemistry of Interstellar Molecular Clouds. Lecture Notes in Physics. No.459. Springer Berlin Heidelberg , pp. 377-379. ISBN 9783540604822. https://resolver.caltech.edu/CaltechAUTHORS:20210217-195625187
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Abstract
The shearing-interferometer originally designed for CSO surface measurements (Serabyn, Masson & Phillips 1991) has been upgraded to operate as a moderate resolution Fourier Transform Spectrometer. With a maximim one-sided travel of 44 cm, the attainable unapodized spectral resolution is 170 MHz. Used with the CSO facility holometric detector, the range of applicability of this FTS is 150-1000 GHz. This instrument has now been used for observations of the transmission of the Earth's atmosphere above Mauna Kea, as well as observations of planetary spectra in the millimeter/submillimeter wavelength ranges. We present a few prefiminary results here.
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| Additional Information: | © Springer-Verlag 1995. This work was supported by NSF grant AST90-15755 and NASA grant NAGW-3303. | |||||||||
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| Subject Keywords: | Giant Planet, Planetary Atmosphere, Atmospheric Transmission, Fourier Transform Spectrometer, Submillimeter Wavelength | |||||||||
| Series Name: | Lecture Notes in Physics | |||||||||
| Issue or Number: | 459 | |||||||||
| DOI: | 10.1007/bfb0102195 | |||||||||
| Record Number: | CaltechAUTHORS:20210217-195625187 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20210217-195625187 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 108102 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Rebecca Minjarez | |||||||||
| Deposited On: | 03 May 2021 18:20 | |||||||||
| Last Modified: | 16 Nov 2021 19:09 |
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