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Analysis of nitric oxide fluorescence bands from high latitude rocket observations of the thermospheric dayglow

Thesis/Dissertation ·
OSTI ID:5572902
Ultraviolet spectra of the Earth's thermospheric dayglow are analyzed. The observations were made on August 10, 1982 from Poker Flats, Alaska, using a rocket-borne spectrometer that measured the wavelength range 1950 to 2170 A. This part of the spectrum is dominated by emissions from the gamma, delta, and epsilon bands of nitric oxide. Column densities of nitric oxide are determined by fitting these fluorescence bands with synthetic spectra. Below 125 km, the (1,0) and (2,0) gamma bands are self-absorbed due to the large NO column densities associated with the auroral zone, particularly when the measurements are made using a horizontally viewing instrument. Three bands of the weak NO epsilon system, (0,1), (0,2), and (0,3), were detected in this region of the spectrum. This is the first time these features have been clearly resolved from spectra of the Earth's dayglow and positively identified with the epsilon system. Because these fluorescently scattered epsilon bands do not connect to the ground vibrational level, they are not affected by self-absorption. With these bands, column densities of nitric oxide were determined to between 100 and 125 km using the epsilon bands.
Research Organization:
Colorado Univ., Boulder (USA)
OSTI ID:
5572902
Country of Publication:
United States
Language:
English