Computational Physics Inc. is developing numerical codes for the
Atmospheric Ultraviolet Radiance Integrated Code (AURIC)
development effort of the Phillips
Laboratory Geophysics Directorate in the area of Ionospheric Impact on
Air Force Systems - Ultraviolet Remote Sensing. The modules will
calculate thermospheric emission spectra and radiances in the
1000 - 6500 Å
wavelength region for dayglow, nightglow, twilight, and
electron aurora, and will account for solar, photoelectron, auroral
electron, and chemical excitation processes, pure and self absorption,
and multiple scattering effects. The modules will provide the
capability to calculate emission spectra as a function of wavelength
and look angle, or provide radiances integrated over specified
wavelength intervals for user-selected viewing geometries. The
integrated codes will provide a powerful tool for computing UV optical
backgrounds, analyzing optical data, and designing sensors. This paper
presents the overall architecture of the codes. The design and
implementation of the photoionization and electron flux modules is
discussed, and examples of the input data and generated output is
shown.
See also:
[Photoelectron plot example]
A comparison of the Feautrier 2-stream transport results (Link),
the AURIC local equilibrium model (no transport), and AE-E photoelectron
measurements [Lee et al., Planet.Space Sci., 28, 947, 1980)].
The Hinteregger et al. [Geophys. Res. Lett., 8, 1147,
1981] solar EUV flux was used in the models.