Physics – Space Physics
Scientist
Physics
Space Physics
Scientist
California Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA
Jet Propulsion Laboratory, MS 183-601, 4800 Oak Grove Drive, Pasadena, CA 91109, USA Institute of Technology, Jet Propulsion Laboratory, Pasadena, Calif.
California Institute of Technology, Jet Propulsion Laboratory, Pasadena
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
JPL / Caltech
jet propulsion laboratory, Pasadena, CA, USA;
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109
Colorado, University, Boulder; JPL, Pasadena, CA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA Pasadena, CA
Jet Propulsion Laboratory
Jet Propulsion Laboratory, Pasadena, CA 91109
Jet Propulsion Laboratory, 4800 Oak Grove Dr., Pasadena, CA, USA
Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 92028
Jet Propulsion Laboratory, 4800 Oak Grove Dr., Pasadena, CA 91109, USA Propulsion Laboratory, 4800 Oak Grove Dr., Pasadena, CA 91109, USA Propulsion Laboratory, Pasadena, California, USA
Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109; National Research Council Research Associate
California Institute of Technology, Pasadena, CA, US
Physics Department, University of California at Santa Barbara, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;
Jet Propulsion Laboratory, Pasadena, California 91109, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
Jet Propulsion Laboratory, 4800 Oak Grove
A Pre-Phobos Assessment of the Composition of the Martian Moons Based on Viking, Mariner 9 and Groundbased Data
A reexamination of important N2 cross sections by electron impact with application to the dayglow - The Lyman-Birge-Hopfield band system and N I (1199.99 nm)
A study of electron impact excitation of NO. I - The vacuum ultraviolet from 40 to 170 nm. II - The middle ultraviolet from 170 to 270 NM
A study of electron impact excitation of NO: The middle ultraviolet from 170 to 270 nm
Airglow emission from Titan during eclipse
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