Hostname: page-component-848d4c4894-pjpqr Total loading time: 0 Render date: 2024-06-19T15:00:57.154Z Has data issue: false hasContentIssue false
  • English
  • Français

8. A brief survey of upper-air spectra

Published online by Cambridge University Press:  14 August 2015

P. M. Millman
P. M. Millman*
Affiliation:
National Research Council, Ottawa, Canada, and Consultant, Avco Everett Research Laboratory, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The atomic multiplets and molecular band systems identified in six categories of upper-air sources are studied. These total 510 multiplets of 38 atoms and ions, and 54 band systems of 27 molecules. The average excitation decreases as one progresses from the sources resulting from the influx of the faster and smaller particles to those produced by the slower and larger objects.

Type
Session 2
Information
Symposium - International Astronomical Union , Volume 33: Physics and Dynamics of Meteors , 1968 , pp. 84 - 90
Copyright
Copyright © Reidel 1968 

References

Bates, D.R. (1960) Physics of the Upper Atmosphere, ed. by Ratcliffe, J. A., Academic Press, New York, pp. 219–353.Google Scholar
Chamberlain, J.W. (1961) Physics of the Aurora and Airglow, Academic Press, New York.Google Scholar
Gatterer, A., Junkes, J., Salpeter, E. W., Rosen, B. (1957) Molecular Spectra of Metallic Oxides, Specola Vaticana, Vatican City.Google Scholar
McKee, C.W. (1966) NASA Technical Note D-3571.Google Scholar
Millman, P.M. (1963) Smithson. Contr. Astrophys., 7, 119.Google Scholar
Moore, C.E. (1945) Contr. Princeton Obs., 20.Google Scholar
Pearse, R.W.B., Gaydon, A.G. (1963) The Identification of Molecular Spectra, 3rd ed., Chapman and Hall, London.Google Scholar