Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Instrumentation and Methods for Astrophysics
Scientist
University of Maryland
University of Maryland, Institute for Physical Sciences and Technology, College Park, MD 20742, USA; NASA Ames Research Center, Space Sciences Division Mail Stop 245-6, Moffett Field, CA 94035, USA of Maryland, IPST, College Park, MD 20742, USA; NASA Ames Research Center, Mail Stop 245-6 Space Sciences Division, Moffett Field, CA 94035, USA Propulsion Laboratory / California Institute of Technology, Mail Stop 183-301 4800 Oak Grove Dr., Pasadena, CA 91109, USA of Physical Sciences and Technology, University of Maryland, College Park, MD 20742, USA; Visiting Scientist at NASA Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035, USA
NASA Ames Research Center, MS 245-6, Moffett Field, CA 94035-1000 ; Institute for Physical Sciences and Technology, University of Maryland, College Park, MD 2074; Also associated with the Institut für Physikalische Chemie, Universität zu Köln, Köln, Germany Propulsion Laboratory
Institute of Physical Sciences and Technology, University of Maryland, College Park, MD, and Molecular Physics Laboratory, SRI International, Menlo Park, CA
Corresponding author; also a senior research scientist at IPST, University of Maryland, College Park, MD 20742, USA.
Institut für Physikalische Chemie, Universität zu Köln, Luxemburger Strasse 116, D-50939 Köln, Germany Ames Research Center, Moffett Field, CA 94035-1000 ; IPST, University of Maryland, College Park, MD 20742; also associated with Institut für Physikalische Chemie, Universität zu Köln, Cologne, Germany
An overview of laboratory studies on the energetic processes in water-rich ices containing organic impurities at outer Solar System temperatures.
Can Biosignatures Be Detected on the Surface of Europa Through Remote Sensing? A Laboratory Study on the Penetration Depths and Reactions of Electrons with Organics
Collisional Removal Rate Constants for N2 (a, υ = 0 and 1) with N2, O2 and O Colliders at 300, 240 and 150 K
Condensed-Phase Photochemical Processes in Titan's Aerosols and Surface: The Role of Longer Wavelength Photochemistry
Consequence of Electron Mobility in Icy Grains on Solar System Objects
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