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Evidence for an OH(u) excitation mechanism of CO sub(2) 4.3 mu m nighttime emission from SABER/TIMED measurements
The SABER instrument on board the TIMED satellite, successfully launched on 7 December 2001, measures the CO sub(2) 4.3 mu m atmospheric emission at day and night, from the troposphere up to the thermosphere, with a near global latitude coverage and with a very high signal-to-noise ratio. SABER has...
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Published in: | Journal of Geophysical Research. D. Atmospheres 2004-05, Vol.109 (D9) |
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Main Authors: | , , , , , , , , , |
Format: | Article |
Language: | English |
Online Access: | Get full text |
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Summary: | The SABER instrument on board the TIMED satellite, successfully launched on 7 December 2001, measures the CO sub(2) 4.3 mu m atmospheric emission at day and night, from the troposphere up to the thermosphere, with a near global latitude coverage and with a very high signal-to-noise ratio. SABER has also three channels near 15 mu m for the measurements of the pressure-temperature structure and two channels around 2.0 and 1.6 mu m, mainly sensitive to the OH(υ |
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ISSN: | 0148-0227 |
DOI: | 10.1029/2003JD004383 |