Engineering topics

Colburn, D.

Publications and source records attributed to Colburn, D..

4 records

NASA NTRS1984

Large, solid particles in the clouds of Venus - Do they exist?

The evidence for solid mode 3 particles in the clouds of Venus is reexamined. The sampling characteristics of the cloud particle size spectrometer (LCPS) are reviewed, and reasons are pointed out for believing that relatively small differences in interpreting the measurements of this instrument could produce systematic errors. It is shown that all of the Pioneer Venus and Venera measurements can be understood if it is assumed that the large particles observed by the LCPS form the tail of the mode 2, H2SO4 size distribution.

Toon, O. B.↗

NASA NTRS1978

Multicolor observations of Phobos with the Viking lander cameras - Evidence for a carbonaceous chondritic composition

The reflectivity of Phobos has been determined in the spectral region from 0.4 to 1.1 micrometers from images taken with a Viking lander camera. The reflectivity curve is flat in this spectral interval and the geometric albedo equals 0.05 + or - 0.01. These results, together with Phobos's reflectivity spectrum in the ultraviolet, are compared with laboratory spectra of carbonaceous chondrites and basalts. The spectra of carbonaceous chondrites are consistent with the observations, whereas the basalt spectra are not. These findings raise the possibility that Phobos may be a captured object rather than a natural satellite of Mars.

Pollack, J. B.↗

NASA NTRS1978

Remote sensing of aerosols in the Martian atmosphere - Implications for terrestrial studies

Data provided by recent spacecraft missions to Mars include determinations of the properties and effects of aerosols suspended in the Martian atmosphere. Comparison of alternative procedures used to remotely sense the aerosol properties as well as analyses of these methodologies may have relevance for analogous procedures being developed to study terrestrial aerosols with satellite-borne sensors. In addition, Martian aerosols appear to have played a role in climate changes that may have terrestrial counterparts. Of particular concern are observations made from the Mariner 9 orbiter spacecraft, which studied Mars during 1971 and 1972, and the Viking orbiter and lander spacecraft, which conducted measurements commencing in the middle of 1976 and continuing through the present. Two global dust storms were observed from their commencement to their demise.

Pollack, J. B.↗

NASA NTRS1977

Properties of aerosols in the Martian atmosphere, as inferred from Viking Lander imaging data

Three types of aerosol were detected from observations of the Martian sky, Phobos, and the sun with the Viking imaging cameras. Atmospheric optical depths were derived from observations of the objects' brightness. Data on the absorption coefficient, mean size, and shape of aerosols were obtained from studies of the sky brightness, using a multiple-scattering computer code. The aerosol types were water ice ground fog, a higher-level ice cloud (polar hood), and soil particles suspended at heights up to 30 km. The properties of each type of aerosol are discussed. The data are subjected to thorough analysis, and the results are summarized.

Pollack, J. B.↗