Azimuth Angle Dependence of Equatorial Ultraviolet Airglow

Details Azimuth Angle Dependence of Equatorial Ultraviolet Airglow Azimuth Angle Dependence of Equatorial Ultraviolet Airglow

Sep 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972natur.239..157q&link_type=abstract

Nature, Volume 239, Issue 5368, pp. 157 (1972).

Physics

Scientific paper

AN ionization chamber and an EUV solar blind photomultiplier were flown to an altitude of 103 km on a Dauphin rocket launched from Kourou, French Guiana (5° N; 35° E), on September 14,1971, at 0020 (local time). The ionization chamber had a 15° field of view and was filled with Cs2 with an MgF2 window; the resulting bandpass is 1150 Å-1250 Å. The photomultiplier, field of view 5°, was enclosed in a sealed box filled with O2 which transmits UV radiation only through 3 windows between 1150 Å and 1250 Å (ref. 1).

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