Intensity of the near infrared OH airglow

Details Intensity of the near infrared OH airglow Intensity of the near infrared OH airglow

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974natur.250..636h&link_type=abstract

Nature, Volume 250, Issue 5468, pp. 636-637 (1974).

Physics

12

Scientific paper

THE OH airglow was studied from the balloon-borne telescope Thisbe on three flights launched in 1971 and 1972 from the NCAR balloon flight station, Palestine, Texas (32°N, 95°W). The principal goal of these flights has been the measurement of the zodiacal light in the near infrared1 with the airglow as a troublesome foreground contribution which had to be determined carefully.

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