Engineering Papers⌕ Search

Engineering topics

Reeves, R. R., Jr.

Publications and source records attributed to Reeves, R. R., Jr..

At least 19 records
All sourcesNASA NTRSDOE OSTI
NASA NTRS1979

Silicon compounds in the Jupiter atmosphere

The formation of colored silicon compounds under nonequilibrium conditions is discussed with reference to the composition of the Jupiter atmosphere. It is shown that many of these reactions produce strongly colored intermediates that are relatively stable and similar in appearance to those observed on Jupiter. It is suggested that the silicon compounds could substantially contribute to the colors observed on Jupiter. The colored intermediates may be the result of relatively rapid amorphous silicon monoxide formation in vertical atmospheric currents in the region near the red spot and in the red spot itself.

Howland, G.↗
NASA NTRS1979

The role of phosphorus in the upper atmosphere of Jupiter

The reaction of elemental phosphorus and H atoms to form PH3 was observed and should be a major factor in the recycling of PH3 in the stratosphere of Jupiter. The formation of PH3 in this manner should predominate at high altitudes where, due to the very low temperatures, reactions that require higher activation energies than these atom reactions cannot occur. At lower altitudes, in the troposphere, the rapid formation of H atoms from the strong absorption of light by NH3 will contribute to phosphine production also in this same manner. Recent experiments have also shown that elemental phosphorus reacts readily with aqueous ammonia to form PH3. This reaction may also be important in the recycling of PH3 in the upper troposphere of Jupiter if water-ammonia clouds, as had been previously thought, exist. Considerations of the coloration of the Great Red Spot have been made based upon the nature of the phosphorus obtained by decomposition of the phosphine.

Howland, G. R.↗
NASA NTRS1978

Measurement of solar radiation at ground level in the region 1950-2150 A using ammonia actinometry

The use of ammonia as an actinometer for measurement of the solar flux in the region 1950-2150 A is presented. The solar flux was found to be 270 million photons/sq cm per sec at ground level in this wavelength interval in an area with minimum overhead ozone concentration. The advantages of this method over previously used methods are discussed, and the results are related to the present estimates of the tropospheric photodissociation rates for the freons CFCl3 and CF2Cl2 by radiation in this wavelength region.

Knoot, P.↗
NASA NTRS1966

Some comments on the Venus temperature.

Interpretations of microwave emission from Venus through experiments in which anomalous signals have been observed in X-band from glow discharges

PLANETARY TEMPERATURE↗