Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Institute of Geophysics and Planetary Physics, University of California at Riverside, Riverside, CA of Geophysics and Planetary Physics, University of California, Riverside, California
Department of Physics & Center for Space Physics and Aeronomic Research, University of Alabama in Huntsville, USA
The University of Alabama in Huntsville, Physics Department / CSPAR, NSSTC Bld., 320 Sparkman Drive, Huntsville, AL 35805, USA
Physics Department and Center for Space Physics and Aeronomic Research, The University of Alabama in Huntsville, AL 35805, USA
Physics Department, University of Alabama in Huntsville, Huntsville, AL 35899, USA ; Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35805, USA ;
Institute of Geophysics and Planetary Physics, University of California, Riverside, CA 92521, USA of Geophysics and Planetary Physics, University of California at Riverside, 1432 Geology Building, 900 University Avenue, Riverside, CA 92521, USA CSPAR, Huntsville, AL, USA; / CSPAR, the University of Alabama in Huntsville, Huntsville, AL, USA; Huntsville, AL, USA; Center for Space Plasma and Aeronomic Research The University of Alabama in Huntsville, Huntsville, AL, USA; U of AL / Huntsville-CSPAR, Huntsville, AL, USA; of Alabama, Huntsville, AL, USA; for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL, USA; Department and CSPAR, University of Alabama, Huntsville, AL, USA; UC-Riverside, 2126 Pierce Hall University of California, Riverside, CA 92521, USA University of California, Riverside, CA 92521, USA University of California
3D Heliospheric Simulations of Heavy Neutral Particles from the Interstellar Medium
An Estimate of the Nearby Interstellar Magnetic Field Using Neutral Atoms
Can IBEX Identify Variations in the Galactic Environment of the Sun using Energetic Neutral Atom (ENAs)?
Charge Exchange Driven Instability of the Heliopause
Comparing various multi-component global heliosphere models
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