The Shuttle SBUV (SSBUV) and NOAA-11 SBUV/2 instruments measured solar spectral UV irradiance during the maximum and declining phase of solar cycle 22. The SSB UV data accurately represent the absolute solar UV irradiance between 200-405 nm, and also show the long-term variations during eight flights between October 1989 and January 1996. These data have been used to correct long-term sensitivity changes in the NOAA-11 SBUV/2 data, which provide a near-daily record of solar UV variations over the 170-400 nm region between December 1988 and October 1994. The NOAA-11 data demonstrate the evolution of short-term solar UV activity during solar cycle 22
The importance of solar irradiance measurements by the Solar Backscatter Ultraviolet, Model 2 (SBUV/...
We use solar spectra obtained by the Ozone Monitoring Instrument (OMI) on board the Aura satellite t...
Trends in atmospheric ozone continue to be an environmental concern. Drifts in satellite observation...
The Shuttle Solar Backscatter Ultraviolet (SSBUV) instrument performs multiple solar spectral irradi...
The principle purpose of this work is to use yearly flights of the Shuttle SBUV/w (SSBUV) instrument...
The NOAA-9 SBEV/2 instrument has made the first regular measurements ot solar UV activity over a com...
The NOAA-11 SBUV/2 spectral solar data have been corrected for long-term instrument changes to produ...
Observations of the Sun by the Solar Backscatter Ultraviolet (SBUV) instrument aboard Nimbus 7 and t...
The purpose of this research is to develop a NOAA-11 SBUV/2 solar spectral irradiance data set which...
The Shuttle Solar Backscatter Ultraviolet (SSBUV) experiment has flown four times since October 1989...
Characterization of temporal and spectral variations in solar ultraviolet irradiance over a solar cy...
The measurements of the solar ultraviolet spectral irradiance by the two Upper Atmosphere Research S...
Observations of temporal variations of the solar UV spectral irradiance over several days to a few w...
Continuous Measurements of the Solar UV have been made by an instrument on the Solar Mesosphere Expl...
Monitoring of the near ultraviolet (UV) solar irradiance is important because the solar UV radiation...
The importance of solar irradiance measurements by the Solar Backscatter Ultraviolet, Model 2 (SBUV/...
We use solar spectra obtained by the Ozone Monitoring Instrument (OMI) on board the Aura satellite t...
Trends in atmospheric ozone continue to be an environmental concern. Drifts in satellite observation...
The Shuttle Solar Backscatter Ultraviolet (SSBUV) instrument performs multiple solar spectral irradi...
The principle purpose of this work is to use yearly flights of the Shuttle SBUV/w (SSBUV) instrument...
The NOAA-9 SBEV/2 instrument has made the first regular measurements ot solar UV activity over a com...
The NOAA-11 SBUV/2 spectral solar data have been corrected for long-term instrument changes to produ...
Observations of the Sun by the Solar Backscatter Ultraviolet (SBUV) instrument aboard Nimbus 7 and t...
The purpose of this research is to develop a NOAA-11 SBUV/2 solar spectral irradiance data set which...
The Shuttle Solar Backscatter Ultraviolet (SSBUV) experiment has flown four times since October 1989...
Characterization of temporal and spectral variations in solar ultraviolet irradiance over a solar cy...
The measurements of the solar ultraviolet spectral irradiance by the two Upper Atmosphere Research S...
Observations of temporal variations of the solar UV spectral irradiance over several days to a few w...
Continuous Measurements of the Solar UV have been made by an instrument on the Solar Mesosphere Expl...
Monitoring of the near ultraviolet (UV) solar irradiance is important because the solar UV radiation...
The importance of solar irradiance measurements by the Solar Backscatter Ultraviolet, Model 2 (SBUV/...
We use solar spectra obtained by the Ozone Monitoring Instrument (OMI) on board the Aura satellite t...
Trends in atmospheric ozone continue to be an environmental concern. Drifts in satellite observation...