Abstract
Molecular oxygen is important in atmospheric models because (1) it is the only major constituent which participates appreciably in chemical reactions with other species, including hydrogen-containing species, (2) it shields all molecules below a certain level from the solar ultraviolet and thereby determines the dissociation rates of the various species, and (3) it is an important source of O atoms through normal dissociation and predissociation.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Blake, A. J., Carver, J. H., and Haddad, G. N.: 1965, ‘Molecular Oxygen Photo-Absorption Cross Sections Between 1050 Å and 2350 Å’, Internal Report, Dept. of Physics, University of Adelaide.
Blake, A. J., Carver, J. H., and Haddad, G. N.: 1966, J. Quant. Spectr. Radiative Transfer, 6, 451–459.
Brace, L. H., Reddy, B. M., and Mayr, H. G.: 1967, J. Geophys. Res. 72, 265.
Brinkmann, R. T., Green, A. E. S., and Barth, C. A.: 1966, ‘A Digitalized Solar Ultraviolet Spectrum’, JPL Tech. Rep. No. 32-951, Jet Propulsion Lab., Pasadena, California.
Detwiler, C. R., Garrett, D. L., Purcell, J. D., and Tousey, R.: 1961, Ann. Geophys. 17, 263.
Donahue, T. M.: 1969, J. Geophys. Res. 74, 1128.
Goody, R. M.: 1964, Atmospheric Radiation, I. Theoretical Basis, Clarendon Press, Oxford, pp. 97–171.
Hesstvedt, E.: 1968, Geofys. Publik. 27, 1.
Hoffman, J. H.: 1967, J. Geophys. Res. 72, 1883.
Hudson, R. D. and Carter, V. L.: 1968, J. Opt. Soc. Am. 58, 1621.
Hudson, R. D., Carter, V. L., and Breig, E. L.: 1969, J. Geophys. Res. 74, 4079.
Hunt, B. G.: 1966, J. Geophys. Res. 71, 1385.
Malitson, H. H., Purcell, J. D., Tousey, R., and Moore, C. E.: 1960, Astrophys. J. 132, 746.
Ogawa, M. and Yamawaki, K. R.: 1970, Appl. Opt. 9, 1709.
Purcell, J. D., Packer, D. M., and Tousey, R.: 1960, ‘The Ultraviolet Spectrum of the Sun’, in Space Res. 1, North-Holland Publ. Co., Amsterdam, pp. 581–589.
Reber, C. A., Cooley, J. E., and Harpold, D. N.: 1967, Trans. Am. Geophys. Union 48, 75.
Shimazaki, T. and Laird, A. R.: 1970, J. Geophys. Res. 75, 3221.
Wilson, N., Tousey, R., Purcell, J. D., Johnson, F. S., and Moore, C. E.: 1954, Astrophys. J. 119, 590.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1971 D. Reidel Publishing Company, Dordrecht-Holland
About this paper
Cite this paper
Brinkmann, R.T. (1971). Photochemistry and the Escape Efficiency of Terrestrial Hydrogen. In: Fiocco, G. (eds) Mesospheric Models and Related Experiments. Astrophysics and Space Science Library, vol 25. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3114-1_5
Download citation
DOI: https://doi.org/10.1007/978-94-010-3114-1_5
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3116-5
Online ISBN: 978-94-010-3114-1
eBook Packages: Springer Book Archive