Physics
Scientist
Department of Geological and Physical Sciences California State University, Chico Chico, California 95926, USA
A Comparison of Venus Cloud Models Determined by Spectroscopic Investigations
An Expanded Theoretical Interpretation of the Venus 1.05-MICRON co, Line and the Venus 0.8226-MICRON h, O Line
Book-Review - Introductory Astronomy Laboratory Exercises
Determination of the properties of the clouds of Venus using quantitatvie spectroscopy.
Moons and planets: An introduction to planetary science W. K. Hartmann. Bogden & Quigley, New York, 1972. 404 pp. Price $12.95
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