Spectroscopy of the EUV (350-1400 A) nightglow

Details Spectroscopy of the EUV (350-1400 A) nightglow Spectroscopy of the EUV (350-1400 A) nightglow

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.5660c&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, July 1, 1984, p. 5660-5664.

Computer Science

Sound

42

Extreme Ultraviolet Radiation, Nightglow, Ultraviolet Spectroscopy, Oxygen Spectra, Particle Precipitation, Satellite Sounding

Scientific paper

The authors present time averaged spectra of the extreme ultraviolet nightglow in the 350 to 1400-Å range at 8-Å resolution. The uplooking spectrum is dominated by geocoronal and interplanetary resonantly scattered solar lines (H I 1216, H I 1026, O II 834, and He I 584 Å). The downlooking spectrum contains O I emission features from the nighttime ionosphere, including several previously unobserved features. In contrast to previously reported observations, no significant N2 Lyman-Birge-Hopfield emissions are evident in the data, and a 2-σ upper limit of 135 R can be placed on this radiation for the time of observations.

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