Physics
Scientist
Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA
Southwest Research Institute, 6220 Culebra Rd., San Antonio, TX 78228, USA
Southwest Research Institute, 6223 Culebra Road, San Antonio, TX 78238, USA
Southwest Research Institute, San Antonio, USA
Jet Propulsion Lab., California Institute of Technology, Pasadena.
University of Bern, Bern, Switzerland
Southwest Research Institute, San Antonio, TX 78238, USA
Max-Planck-Inst. für Aeronomie, Katlenburg-Lindau, Germany
Lockheed Missiles and Space Co., Palo Alto, CA.
Southwest Research Institute, San Antonio, Texas, USA
JPL
Southwest Research Institute, Division of Space Science and Engineering 9503 W Commerce, San Antonio, TX 78227-1301, USA
Southwest Research Institute, PO Drawer 28510 Division 15, BLDG. 178, San Antionio, TX 78228-0510, USA
Southwest Research Institute, P.O. Drawer 28510, San Antonio, TX 78228-0510, USA
Southwest Research Institute, PO Drawer 28510, San Antonio, TX 78228-0510, United States
Jet Propulsion Lab., California Institute of Technology, Pasadena, CA, US
Lockheed Aircraft Corp., Palo Alto, Calif.
Bern Univ., Switzerland
JPL, Pasadena, CA
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive Pasadena, CA 91109-8099, USA
Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78254, USA Research Institute, 6220 Culebra Road, San Antonio, TX 78238-5166, USA
Southwest Research Institute, San Antonio, TX
Southwest Research Institute, PO Drawer 28510, San Antonio, Texas 78228, USA
Southwest Research Institute, 6220 Culebra Rd., San Antonio, TX 78238, USA
Southwest Research Institute;, Jet Propulsion Laboratory
California Institute of Technology, Jet Propulsion Laboratory, Pasadena, Calif.
Southwest Research Institute,
A Comparison of CAPS Composition Measurements of the Plasma near Enceladus with Predictions of a Chemical Model
A comprehensive program for countermeasures against potentially hazardous objects (PHOs)
A different view of plasma flow inside P/Halley
A Multi-fluid Model of Enceladus: Plume Interactions With Saturn's Local Magnetospheric Flow
A New Laboratory Technique for High Resolution Absorption Spectroscopy over Ultra Long Paths
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