The EUV dayglow at high spectral resolution

Details The EUV dayglow at high spectral resolution The EUV dayglow at high spectral resolution

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95.4113m&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, April 1, 1990, p. 4113-4127.

Computer Science

Sound

30

Dayglow, Extreme Ultraviolet Radiation, Oxygen Spectra, Rocket Sounding, Spectral Resolution, Midlatitude Atmosphere, Nitrogen, Terrestrial Radiation

Scientific paper

Rocket observations and spectra of the dayglow spectrum of the terrestrial atmosphere between 840 and 1860 A are studied. Three bands of the N2 c-prime 4 system are seen clearly resolved in the dayglow. Analysis of high-resolution N2 Lyman-Birge-Hopfield data shows no anomalous vibrational distribution as has been reported from other observations. Altitude profiles of the observed O and N2 emissions demonstrate that the MSIS-83 model O and N2 densities are appropriate for the conditions of the rocket flights.

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