Physics
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988angeo...6..417d&link_type=abstract
(IAMAP and International Commission on the Meteorology of the Upper Atmosphere, Workshop on Downward Penetration of Solar Activi
Physics
20
Solar Radiation, Solar Terrestrial Interactions, Stratosphere, Ultraviolet Spectra, Nimbus 7 Satellite, Power Spectra, Solar Backscatter Uv Spectrometer, Solar Cycles, Solar Rotation
Scientific paper
Solar-rotation induced variations of solar UV observations from the Solar Backscatter UV instrument on the Nimbus-7 satellite are highly uniform in temporal shape in the 175-285 nm range. Considering this UV temporal uniformity and the averaging effects of the multiple wavelength dependence of the stratospheric response, solar UV flux changes may be expressed as a product of a wavelength dependent function U(lambda) and a time dependent function V(t). The Mg II center-to-wing ratio is weak in 13-day periodicity relative to the rest of the 175-285-nm UV flux. The 205-nm solar UV flux is recommended for determining the short-term variations of V(t), and the Mg II center-to-wing ratio is recommended for the intermediate (several months) and long-term (years) variations of V(t).
No associations
LandOfFree
Uniformity in solar UV flux variations important to the stratosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Uniformity in solar UV flux variations important to the stratosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Uniformity in solar UV flux variations important to the stratosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1693440