Satellite observations of the oi 1304, 1356 and 1641 Å dayglow and the abundance of atomic oxygen in the thermosphere

Author:

Conway R.R.,Meier R.R.,Huffman R.E.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference27 articles.

1. The UV dayglow, OI emissions at 989, 1027, 1152, 1304 and 1356 Å;Anderson;Geophys. Res. Lett.,1980

2. Self-absorption of the N2 Lyman-Birge-Hopfield bands in the far ultraviolet dayglow;Conway;J. geophys. Res.,1982

3. Photoabsorption and photoionization cross sections of O, O2 and N2 for photoelectron pro-duction calculations: a compilation of recent laboratory measurements;Conway;NRL Memo Report 6155,1987

4. The far ultraviolet vehicle glow of the S3-4 satellite;Conway;Geophys. Res. Lett.,1987

5. The ultraviolet dayglow at solar maximum, far UV spectroscopy at 3.5 Å resolution;Eastes;J. geophys. Res.,1985

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