Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
Scientist
Brown University, Department Geological Sciences Box 1846, Providence, RI 02912, USA Propulsion Laboratory, California Institute of Technology, Mail Stop 183-301, 4800 Oak Grove Drive, Pasadena, California 91109, USA
JPL, 4800 Oak Grove, Pasadena, CA 91109, USA
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove, Pasadena, CA 91109, USA Propulsion Laboratory, Pasadena, California, USA
Jet Propulsion Laboratory, Caltech, Pasadena, CA 91109 Propulsion Laboratory / Caltech, MS 183-301 4800 Oak Grove Dr., Pasadena, CA 91109, USA Propulsion Laboratory / Caltech, MS183-301 4800 Oak Grove Dr., Pasadena, CA 91109, USA Propulsion Lab, Caltech, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Department of Civil Engineering and Geological Sciences, University of Notre Dame, Notre Dame, Indiana 46556, USA
JPL, Caltech, Pasadena, CA 91109
Division of Geological Sciences, Califronia Institute of Technology, Pasadena, CA 91125, USA
Department of Geological Sciences Brown University, Box 1846, EM: Ralph_ Providence, RI 02912, USA
Jet Propulsion Laboratory, Pasadena, CA 91109, USA
Geological Sciences, Box 1846 Brown University, Providence, RI 02912, USA
JPL, 4800 Oak Grove Dr., Pasadena, CA 91001 Caltech, Pasadena, 91109
Department of Civil Engineering and Geological Sciences, University of Notre Dame, Notre Dame, Indiana, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
Jet Propulsion Laboratory, California Institute of Technology, MS 183-301, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Jet Propulsion Laboratory, California Institute of Technology, MS 183-401, 4800 Oak Grove Drive, Pasadena, California 91109, USA
Jet Propulsion Laboratory, MS 183-30, 4800 Oak Grove Dr., Pasadena, CA 91109,
2 Pallas and 10 Hygiea in the 3-μm spectral region
A Laboratory-based Model for Estimating Absolute H2O Content of Minerals Using VIS-NIR Spectroscopy
A large diversity of hydrated minerals formed from interaction with hydrothermal fluids in Noctis Labyrinthus, Mars.
A Modified CIPW Norm Calculation for Lunar Mare Basalts
An experimental approach to clay mineral formation on Mars
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