Ultraviolet radiation of Venus in the 300-1657-A wavelength range from Venera 11 and 12 data /preliminary results/

Details Ultraviolet radiation of Venus in the 300-1657-A wavelength range from Venera 11 and 12 data /preliminary results/ Ultraviolet radiation of Venus in the 300-1657-A wavelength range from Venera 11 and 12 data /preliminary results/

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..772k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, Sept.-Oct. 1979, p. 772-779. In Russian.

Astronomy and Astrophysics

Astronomy

1

Planetary Radiation, Ultraviolet Radiation, Venera Satellites, Venus Atmosphere, Astronomical Spectroscopy, Atmospheric Density, Boltzmann Distribution, Carbon Dioxide Concentration, Collimators, Cosmic Rays, Exosphere, Helium Atoms, Hydrogen Atoms, Numerical Integration, Photomultiplier Tubes, Radiant Flux Density, Scattering, Spectroscopic Telescopes

Scientific paper

Spectrometers aboard Venera 11 and 12 have measured UV radiation
scattered in the upper atmosphere of Venus. This paper discusses
preliminary results of these measurements, and gives attention to
scattered radiation intensity, the intensity of Lyman-alpha radiation,
and the intensity of the He I 584-A line near the illuminated limb.

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