Solar variability in the spectral range 2350-2870 A

Details Solar variability in the spectral range 2350-2870 A Solar variability in the spectral range 2350-2870 A

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....88.6797h&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 88, Aug. 20, 1983, p. 6797-6799.

Physics

13

Irradiance, Solar Radiation, Spectral Energy Distribution, Ultraviolet Radiation, Balloon-Borne Instruments, Line Spectra, Magnesium, Stratosphere, Ultraviolet Spectrometers

Scientific paper

Between April 1977 and April 1981, four balloon flights of a solar ultraviolet spectrometer were made to altitudes near 40 km in the stratosphere. Analysis of these measurements shows that the solar irradiance in the wavelength range 2350-2870 A has been constant within + or - 7 percent over this period. The central emission cores of the Mg II resonance lines increased in intensity by about 20 pecent over the same time period.

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