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GOMOS was first proposed in 1988 as an
Announcement of Opportunity instrument dedicated to be a part of the Earth Observation Polar Platform Mission, the former name of Envisat. In 1992 it was decided that GOMOS would be developed as a
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from South Pole to North Pole. Data acquired on dark limb (night-time) are of better quality than on bright limb (day-time) because of a smaller perturbation by background light.
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are used to correct star scintillation perturbations and to determine high vertical resolution temperature profiles.
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launched 1 March 2002. It is the first space instrument dedicated to the study of the
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Global latitude coverage is obtained with up to 40 stellar occultations per
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and related species in the middle atmosphere (15 to 100 km).
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74:spectral domain is used for the determination of
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17:Global Ozone Monitoring by Occultation of Stars
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34:of the Earth by the technique of stellar
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38:. The spectrum of stars in the
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200:. You can help Knowledge by
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52:electromagnetic spectrum
152:Official ESA GOMOS page
252:Spacecraft instruments
196:-related article is a
23:on board the European
140:European Space Agency
142:-funded instrument.
162:2020-02-18 at the
66:Instrument details
257:Outer space stubs
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19:(GOMOS), is an
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164:Wayback Machine
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146:External links
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202:expanding it
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70:The 250-680
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194:spaceflight
120:photometers
101:temperature
56:climatology
40:ultraviolet
36:occultation
241:Categories
157:GOMOS page
32:atmosphere
21:instrument
25:satellite
160:Archived
97:aerosols
46:and the
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44:visible
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192:- or
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