Physics
Scientist
UCLA-IGPP, Box 951567, Los Angeles, CA 90095-1567, USA
IGPP-UCLA, 405 Hilgard Avenue, Los Angeles, CA 90095-1567, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles 405 Hilgard Ave., Los Angeles, CA 90095-1567, USA
Institute of Geophysics and Planetary Physics, University of California Los Angeles, 405 Hilgard Ave, Los Angeles, CA 90095-1567, USA
Institute of Geophysics and Planetary Physics, University of California Los Angeles, 405 Hilgard Avenue, Los Angeles, CA 90095-1567, USA
IGPP-UCLA, 405 Hilgard Ave., Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics, University of California Los Angeles, 405 Hilgard Ave., Los Angeles, CA 90095, USA
UCLA-IGPP, 405 Hilgard Ave, Los Angeles, CA 90095-1567, USA
Institute of Geophysics and Planetary Physics, UCLA, 405 Hilgard Avenue, Los Angeles, CA 90095, USA of Geophysics and Planetary Physics, UCLA, 405 Hilgard Avenue, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, Los Angeles, California, USA
Insititue of Geophysics and Planetary Phsyics, University of California, Los Angeles 405 Hilgard Ave., Los Angeles, CA 90095-1567, USA
IGPP / UCLA, 405 Hilgard Avenue, Los Angeles, CA 90095-1567, USA
IGPP, UCLA, Los Angeles, CA 90095-1567, USA
Institute of Geophysics and Planetary Physics, University of California at Los Angeles, Los Angeles, CA 90095-1567, USA
UCLA-IGPP, 405 Hilgard Avenue, Los Angeles, CA 90095-1567, USA
UCLA - IGPP, 405 Hilgard Ave., Los Angeles, CA 90095
UCLA-IGPP, Box 951567 3870 Slichter Hall 405 Hilgard Ave., Los Angeles, CA 90095-1567, USA mosta
A comparison of solar wind and ionospheric plasma contributions to the September 24 25, 1998 magnetic storm
A new convection state at substorm onset: Results from an MHD study
A simulation study of particle energization observed by THEMIS spacecraft during a substorm
A stochastic sea: The source of plasma sheet boundary layer ion structures observed by Cluster
Acceleration of Electrons from the Solar Wind to the Inner Magnetosphere During Storms
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