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Radiometer for the measurement of water vapor in the upper atmosphere from space.

Abstract:
We describe the design, the development, and the calibration of a radiometer to measure water vapor abundance in the middle atmosphere, using the solar occultation technique from an orbiting platform. The use of gas cells containing water vapor and carbon dioxide leads to a relatively simple, but sensitive, design. This radiometer is shown to be capable of detecting water vapor in the mesosphere, where, because of dissociation by the Sun, the amounts are very small, of the order of 1 part per 10(6) or less. A flight version of the instrument will be launched in 1992 on board the European Retrievable Carrier space platform, and the data will be employed for a better understanding of the Earth's water budget.
Publication status:
Published

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Publisher copy:
10.1364/ao.32.006764

Authors

More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author


Journal:
Applied optics More from this journal
Volume:
32
Issue:
33
Pages:
6764-6776
Publication date:
1993-11-01
DOI:
EISSN:
1539-4522
ISSN:
0003-6935


Language:
English
Keywords:
Pubs id:
pubs:1900
UUID:
uuid:122658da-eaa6-4a27-ae13-1786a4bb7bfa
Local pid:
pubs:1900
Source identifiers:
1900
Deposit date:
2012-12-19
ARK identifier:

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