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Type of Document	Dissertation
Author	Saint-Amand, Pierre
URN	etd-05122003-113804
Persistent URL	http://resolver.caltech.edu/CaltechETD:etd-05122003-113804
Title	A possible relation between the night airglow and the ionosphere
Degree	PhD
Option	Geological and Planetary Sciences
Advisory Committee	Advisor Name Title Unknown Committee Member
Keywords	None
Date of Defense	1953-01-01
Availability	unrestricted
Abstract (1) It has been found that the diurnal variation of the 6300-6364 Angstrom OI radiation is similar to the diurnal variation of the electron density of the F Layer of the ionosphere. It has been suggested that this similarity is not incidental, and the two phenomena are closely related to each other. The factor of proportionality changes with the seasons. (2) It has been found further that the diurnal variation of the intensity of the 5577 OI radiation is similar to the diurnal variation of the height of the F layer. It is postulated that the 5577 radiation takes place within a region which shares in the vertical movements of the F layer. (3) It has been found also that the intensity of the 6300-6364 radiation changes when the height of the F region changes. (4) Heights calculated by the method of Van Rhijn for the 6300-6364 radiation fall within the height range of the F layer. Those calculated by this method for the 5577 radiation fall at the base of the F region. The independent identification of the radiation with the F region lends confidence to height values of the emitting regions calculated by Roach, Barbier and others. (5) The mechanisms of excitation producing the 5577 and 6300 radiations appear to be different. There is also little evidence for production of the redlines by cascading of electrons from the energy levels producing the green line. (6) The instrumentation used in measuring the intensity of the nightglow is discussed in detail.
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