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Wagener, Richard

Publications and source records attributed to Wagener, Richard.

7 records
All sourcesNASA NTRSDOE OSTI
DOE OSTI2022

csphothybv3: A hybrid sky radiance scan scenario version 3 data

This hybrid scan starts at the position of the Sun and first follows the great circle that is orthogonal to the Principal Plane until it reaches a viewing zenith angle of 75 degrees and then follows the almucantar keep that viewing zenith angle constant. The scan is then repeated in the opposite azimuth direction. This mode was designed to optimize the range of scattering angles and significantly improves the retrieval of inversion parameters especially at low solar zenith angles.

54 ENVIRONMENTAL SCIENCES↗
NASA NTRS1991

Titan's surface and troposphere, investigated with ground-based, near-infrared observations

Characterizations are presently made of Titan's haze, cloud, surface albedo, and atmospheric H2 abundance on the bases of 4000-5000/cm near-IR spectrum and points from the Fink and Larson (1979) 4000-12,500/cm spectrum. The strength of solar radiation absorption varies significantly with wavelength, facilitating a probing of the various atmospheric levels down to the surface. The present observations suggest the existence of an optically thin CH4 cloud layer, as well as haze and cloud optical depths sufficiently small for surface sensing at 4900, 6250, and 7700/cm. The albedos at these wavenumbers indicate the dominant surface material to be 'dirty' water ice.

Griffith, Caitlin A.↗
NASA NTRS1991

UV spectroscopy of Titan's atmosphere, planetary organic chemistry and prebiological synthesis. II - Interpretation of new IUE observations in the 220-335 nm range

The theoretical model developed by McKay et al. (1989) to characterize the size distribution, thermal structure, and chemical composition of the stratospheric haze of Titan is applied to new 220-335-nm albedo measurements obtained with the long-wavelength prime camera of the IUE during August 1987. Data and model predictions are presented in extensive graphs and discussed in detail. It is shown that a simple model with particles of one size at a given altitude does not accurately reproduce the observed features in all spectral regions, but that good general agreement is obtained using a model with a uniformly mixed layer at 150-600 km and a bimodal distribution of small 'polymer' haze particles (radius less than 20 nm) and larger haze particles (radius 100-500 nm). The number densities implied by this model require, however, a mechanism such as electrostatic charging or reaction kinetics to inhibit coagulation of the smaller particles.

Courtin, Regis↗
NASA NTRS1990

The ultraviolet continuum albedo of Uranus

A radiative transfer code explicitly treating the Raman scattering of solar protons by H2 is presently used to analyze the Uranus geometric albedo in the 2000-5000 A range. The Baines and Bergstralh (1986) baseline model used reproduces the geometric albedo peak produced by Raman scattering filling of solar absorption line cores, but is found to be excessively bright for wavelengths below 2400 A. This discrepancy is resolvable through inclusion of an absorbing stratospheric haze layer, and results are thereby obtained which are consistent with the Pollack et al. (1987) model, in which aerosols are generated stratospherically through photochemical effects on hydrocarbons.

Cochran, William D.↗
NASA NTRS1988

Observations of Neptune and Uranus below 2000 A with the IUE

The present IUE observations of Neptune, together with improved observations of Uranus below 2000 A, indicate excellent agreement between the UV-derived C2H2 abundance and that obtained from independent IR data for Uranus, while for Neptune, the derived IUE C2H2 abundances differ from IR spectra by orders of magnitude. Attention is accordingly given to aspects of IR modeling requiring modification. The agreement for Uranus may be due to approximately global uniformity, while the disagreement for Neptune may have its basis in such spatial variations as a warm summer pole, as well as in inaccuracies in current model temperature profiles.

Caldwell, John↗
NASA NTRS1988

Strong north/south asymmetry in the Jovian stratosphere

Trailed spectra of standard B stars have been used as the 'flat' field light source for spatial calibration of IUE large-aperture observations of the north and south polar regions of Jupiter. Longward of 2000 A, the south polar spectrum is lower than the north polar one by a factor of 2.5; shortward of 2000 A, strong C2H2 absorption appears in both north polar and midlatitude spectra, while neither continuum nor band absorption features of C2H2 appear in the south polar spectrum. The very low reflectivity of the south polar region calls for the presence of a stratospheric absorber at pressures lower than 10 mbar.

Wagener, Richard↗