Determination of Molecular Dissociation Rates from Measurements of Scattered Solar Ultraviolet Light
Document Type
Article
Journal/Book Title/Conference
Journal of Geophysical Research
Issue
98
Publication Date
1-1-1993
First Page
9011
Last Page
9022
Abstract
Scattereds olaru ltravioletl ight in the spectral region from 250 to 320 nm was measured from a balloon platform at altitudes ranging from 14.5 to 38.8 km with a wavelengthr esolutiono f approximately0 .3 nm and an accuracyin determiningth ew avelengthp ositiono f 0.5 nm. We usedt heses catterd atat o comparea ndv alidatea single scatteringm odel developedf or this purpose. Using these semi-empiricarl esults,w e constructedth e singles cattered component of the ultraviolet irradiance as a function of height and wavelength. From these data, it is possible to determinet he percentaged issociationra te of a variety of speciesd ue to scatteredu ltravioletr adiation. Theser esults are presenteda s a ratio of intensitiesR = I•/(I0+I0, where I• is the first order scatteringa nd I0 is the direct attenuated radiation from the sun. The attenuated direct radiation from the sun can be multiplied by the factor 1/(l-R), the Rayleigha mplificationr atio usedb y Nicolet et al. (1982), to include the contribution to the irradiance from first order scattered light. The results are multiplied by a cross sectiono f the speciesu nder considerationto obtain the dissociationra tes. Ozoneo verburdena nd an approximate ozone particle density altitude profile are obtained when validating the single scatter model.
Recommended Citation
Montierth, K. V.; Baker, K. D.; Jensen, L. L.; and Megill, L. R., "Determination of Molecular Dissociation Rates from Measurements of Scattered Solar Ultraviolet Light" (1993). Space Dynamics Laboratory Publications. Paper 91.
https://digitalcommons.usu.edu/sdl_pubs/91