Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
NASA / Goddard Space Flight Center Greenbelt, MD 20771, USA
NASA / GSFC, Greenbelt, MD, USA
NASAGSFC, MD 20771, Greenbelt, USA
NASA Goddard
University of Maryland
NASA, Goddard Space Flight Center, Laboratory for Planetary Atmospheres, Greenbelt, Md.
National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, MD.
NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
NASA, Goddard Space Flight Center, Greenbelt, MD
Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, USA
NASA, Goddard Space Flight Center, Laboratory for Extraterrestrial Physics, Greenbelt, MD
Goddard Space Flight Center / University of Maryland
Goddard Space Flight Center / NASA, Greenbelt, MD, USA
Astronomy, University of Maryland, College Park, MD, USA
NASA Goddard Space Flight Center
NASA / GSFC, Greenbelt, Maryland, USA
Department of Astronomy, University of Maryland at College Park, College Park, MD 20742, USA; Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Goddard Space Flight Center, Greenbelt, MD 20771, USA ; Department of Astronomy, University of Maryland, College Park, MD 20742, USA
University of Maryland, Department of Astronomy, College Park, MD 20742, USA
NASA / Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, USA; Department of Astronomy, University of Maryland, College Park, MD 20742, USA
NASA's GSFC
Department of Astronomy, University of Maryland, College Park, MD 20742, USA
Department of Astronomy, University of Maryland, College Park, MD 20742, USA of Astronomy, University of Maryland, 20742, College Park, MD, USA
University of Maryland, Department of Astronomy, College Park, MD 20742, United States
A heuristic approach to examining volatile equilibrium at Titan's surface.
A heuristic approach to examining volatile equilibrium at Titan's surface.
An intense stratospheric jet on Jupiter
Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission II: Aerosol extinction profiles in the 600-1420 cm-1 spectral range
Aromatic Structures in Simulated Titan Aerosol
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