Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Chicago, University, Chicago, IL
Chicago, University, Chicago, IL; California, University, Berkeley, CA
California, University, Berkeley, CA; Chicago, University, Chicago, IL
NASA / JPL
Jet Propulsion Laboratory
JPL, Pasadena, CA 91109 USA
Jet Propulsion Laboratory, Pasadena, CA 91109
Chicago Univ., IL.
Jet Propulsion Laboratory, California Institute of Technology, MS 169-327 4800 Oak Grove Dr., Pasadena, CA 91109, USA
Jet Propulsion Laboratory, MS 169-327, Pasadena, CA 91109, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
Chicago, University, IL
Jet Propulsion Laboratory, Pasadena, California, USA
JPL / Caltech, Pasadena, CA, USA;
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;
Jet Propulsion Laboratory, Pasadena, CA, USA;
JPL, Pasadena, CA, USA;
Jet Propulsion Laboratory / Caltech, Pasadena, CA, USA;
Jet Propulsion Laboratory, Caltech, Pasadena, CA, USA;
California, University, Berkeley, Calif.
Jet Propulsion Laboratory, California Institute of Technology, Pasadena CA 91109
Jet Propulsion Laboratory, California Institute of Technology, M.S. 169-327 4800 Oak Grove Dr., Pasadena, CA 91109, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109
Jet Propulsion Laboratory, Pasadena, CA 91009, USA
Jet Propulsion Laboratory, MS 169-327, Pasadena, CA 91109, USA Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena CA 91190
Jet Propulsion Laboratory, Pasadena, Ca
A cosmic-ray age based on the abundance of Be-10
A measurement of the isotopic composition of galactic cosmic ray carbon, nitrogen and oxygen
A New Evaluation of the Galactic Cosmic Ray Radiation Dose In Interplanetary Space
A New Model of the Galactic Cosmic Ray Radiation Environment at 1 AU based on ACE Measurements
A Novel Technique to Determine Ionic Charge States in Large Solar Particle Events
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