Radii, albedos, and 20-micron brightness temperatures of Iapetus and Rhea.
Explore the source record for details and available documents.
Murphy, R. E.↗
Engineering topics
Morrison, D.
Publications and source records attributed to Morrison, D..
20-micron fluxes of bright stellar standards.
Explore the source record for details and available documents.
Simon, T.↗
Temperatures of Titan and the Galilean satellites at 20 microns.
Determination of the effective temperatures of the satellites by means of broad-band observations made at Mauna Kea in 1971. The temperatures of the Galilean satellites are in fair agreement with observations at shorter wavelengths and with theory. The 20-micron flux of Titan is nearly an order of magnitude lower than expected, suggesting either low surface emissivity or high atmospheric opacity between 18 and 25 micron. Hydrogen could produce the required opacity, but the abundance needed is large.
Morrison, D.↗
Thermal inertia of Ganymede from 20-micron eclipse radiometry
Ganymede thermal inertia data from simultaneous visual photometry and IR radiometry observations during 17 March 1971 eclipse
Beery, J. G.↗
Venus - Determination of atmospheric parameters from the microwave spectrum
Venus atmosphere composition and structure from microwave spectrum, noting surface pressure and temperature and water vapor
Morrison, D.↗
Thermophysics of the planet Mercury
Mercury microwave and IR observations interpreted for thermophysical models for planetary subsurface, discussing rotation and heating
Morrison, D.↗
Venus - Determination of atmospheric parameters from the microwave spectrum
Venus atmospheric parameters from microwave spectrum, discussing brightness temperature, carbon dioxide content, opacity, water vapor, dust and models
Morrison, D.↗
The microwave spectrum of Mercury
Mercury disk temperature from microwave spectrum analysis, proposing subsurface greenhouse effect
Klein, M. J.↗
Martian temperatures and thermal properties
Martian surface temperature distributions based on IR scans of disk compared with predictions of thermal properties
Morrison, D.↗
Venus - Absence of a phase effect at a 2- centimeter wavelength.
Observations of Venus at 15.4 GHz establishing upper limit for brightness variation with phase angle
Morrison, D.↗
Thermal models and microwave temperatures of the planet Mercury
Physical properties of epilith of Mercury from comparison of infrared and microwave brightness temperatures with theoretical thermal models
Morrison, D.↗
Martian surface temperatures
Reduction of infrared scan data on Martian surface temperatures
Morrison, D.↗
Hypersensitization of infrared-sensitive photographic emulsions.
Hypersensitization methods for IR sensitive photographic emulsions investigated for combined speed increase and density uniformity in astronomical photometry
Greenberg, E. H.↗
On the interpretation of Mercury observations at wavelengths of 3.4 and 19 mm.
Microwave observations of Mercury at 3.4 and 19 mm, interpreting brightness temperature variation with phase angle with basically lunar model
Morrison, D.↗
The microwave phase effect of Mercury.
Mercury brightness temperatures from contact conduction and radiative transfer equation solutions, noting dependence on heliocentric longitude and phase angle
Morrison, D.↗