skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Study of a sector spectrophotometer and auroral O/sup +/(2P--2D) emissions

Technical Report ·
OSTI ID:7327938

The metastable OH(2P--2D) auroral emission was investigated. The neighboring OH contaminants and low intensity levels of the emission itself necessitated the evolution of an instrument capable of separating the emission from the contaminants and having a high sensitivity in the wavelength region of interest. A new type of scanning photometer was developed, and its properties are discussed. The theoretical aspects of auroral electron interaction with atomic oxygen and the resultant O/sup +/(2P--2D) emissions were examined in conjunction with N2/sup +/1NEG emissions. Ground based measurements of O/sup +/(2P-2D) auroral emission intensities were made using the spatial scanning photometer (sector spectrophotometer). Simultaneous measurements of N2/sup +/NEG/sub 1,0/ emission intensity were made in the same field of view using a tilting photometer. Time histories of the ratio of these two emissions made in the magnetic zenith during auroral breakup periods are given. Theories of I/sub 73/1/sub 9//I/sub 4278/ of previous investigators were presented. A rocket measurement of N/sub 2//sup +/1NEG/sub 0,0/ and O/sup +/(2P--2D) emission in aurora was examined in detail and was found to agree with the ground-based measurements. Theoretical examination resulted in the deduction of the electron impact efficiency generating O/sup +/(2P) and also suggests a large source of O/sup +/(2P) at low altitude. A possible source is charge exchange of N/sup +/(1S) with O I(3P). (auth)

Research Organization:
National Aeronautics and Space Administration, Huntsville, Ala. (USA). George C. Marshall Space Flight Center
OSTI ID:
7327938
Report Number(s):
N-76-18725; NASA-TN-D-8143; TRN: 77-003856
Country of Publication:
United States
Language:
English