Gloersen, P., Nordberg, W., Schmugge, T. J., Wilheit, T. T., and Campbell, W. J., 1973b, Microwave signatures of first-year and multiyear sea ice: Jour. Geophys. Research, v. 28, no. 18, p. 3564-3572. Hammack, James C., 1977, Landsat goes to sea: Photogrammetric Eng. and Remote Sensing, Vol. XLIII, no. 6, p. 683-691. Harris, G. and Graham, L. C., 1976, Landsat-radar combination; 13th Congress Int. Soc. Photogramm. Comm. VII, Helsinki, Finland. Hemphill, W. R., Stoertz, G. E., Markle, D. A., 1969, Remote sensing of Internat. Symposium on Remote Sensing of luminescent materials: Environment, 6th, Ann Arbor, Mich. 1969, Proc., p. 565-585. Hemphill, W. R., and Watson, R. D., Bigelow, R. C., and Hessen, T. D., 1977, Measurement of luminescence of geochemically stressed trees and other materials, U.S. Geol. Survey Prof. Paper 1015, p. 93-112, 14 figs., 9 tables. Kleinkopf, M. D., de la Fuente D., M. F., Raines, G. L., and Peterson, D. L., 1977, Geophysical Research in Porphyry Copper Exploration, Northern Mexico: Geol. Soc. of America, Abstracts with Program, Rocky Mountain Section, vol. 8, no. 5, p. 595. REFERENCES Adey, A. W., 1972, Microwave radiometry for remote sensing from aircraft and spacecraft, in Resource Satellites and Remote Airborne Sensing Aviation Week and Space Technology, 1977, Special reports: Satellite technology serving Earth: Special Issue of Aviation Week and Space Technology, v. 107, no. 16 (17 Oct 77), p. 9 and p. 40-166. . Basharinov, A. E., Borodin, L.' F., and Shutko, A. M., 1974, Passive Sensing of Environment, 9th, Ann Arbor, Mich. 1974 Proc., p. 363-367. Carter, W. D., Kowalik, W. S., Ballon A., Raul and Brockmann, C., (in press), Mapping Andean Salar deposits by Landsat radiance values: Open file Rept., 41 p. Deutsch, Morris, 1974, Survey of remote-sensing applications: Water Deutsch, Morris, Strong, A. E., and Estes, J. 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C., and Anderson, A., 1975, Photo-optical contrast stretching of Landsat data for multidisciplinary analyses of the Lake Ontario Basin: Proc. Third Canadian Symp. on Remote Sensing, September 1975, p. 173–193, Canadian Aeronautics and Space Institute, Ottawa. Ferrigno, J. G., and Williams, R. S., Jr., 1977, Satellite image atlas of glaciers: Summary of a proposed paper for the International Glaciological Society's "Symposium on Dynamics of Large Ice Masses," Carleton University, Ottawa, Canada, 21-25 August 1978, 6 p. (preprint). Fischer, William A., Lathram, Ernest H., 1973, Concealed structures in Arctic Alaska identified on ERTS-1 imagery: 011 & Gas Jour., May 28, 1973, 5 p. Gloersen, P., Wilheit, T. T., Chang, T. C., Nordberg, W., and Campbell, W. J., 1973a, Microwave maps of the polar ice of the Earth: NASA Goddard Space Flight Center, X-65-2-73-269. 24-215 O -78 - 31 Moon Current plans for additional lunar exploration are uncertain. The Lunar Polar Orbiter (LPO), a spacecraft primarily designed for systematic geochemical measurements of the surface, is being studied. Large jumps in knowledge could occur from future planetary exploration with respect to Venus and the satellites of the outer planets (Jupiter, Saturn) which are at present largely unknown. The next few years will see a rapid expansion of our knowledge of the solar system. The major events anticipated are as follows: Mars In addition to the Viking missions previously cited, high public interest in Viking has stimulated recommendations for another Mars mission in 1984. Rovers with a 100 km roam radius and an orbiter equipped mainly with geochemical sensors and penetrators, and possibly a sample return, are being considered. Venus A Venus orbiter imaging radar (VOIR) is needed to study the surface features of this planet. This radar has been given the highest ranking by most science advisory groups and will return high resolution images (less than 1 km) of most of the planet. Because Venus is closest to the Earth in size and composition, this mission, and the 1978 radar mission to measure mechanical properties of the Venusian surface, have particular interest to terrestrial geologists. Two GS scientists are members of the science team. Jupiter Two Voyager spacecraft are presently on their way to Jupiter and Saturn. The satellites of those planets range widely in density and surface properties, and considerable variations in the geology are anticipated. Voyager will return several thousand pictures for study and analysis. A subsequent mission to orbit Jupiter would provide a more systematic set of observations than will be possible from Voyager. Saturn The Voyagers, launched in 1977 for an encounter with Jupiter, will continue on for an encounter with Saturn in 1983. |