Physics – Space Physics
Scientist
Physics
Space Physics
Scientist
UC Berkeley, Space Sciences Laboratory, MC 7450 7 Gauss Way, Berkeley, CA 94720-7450, USA
SSL, UC Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450, USA
UC Berkeley, Space Sciences Lab 7 Gauss Way, Berkeley, CA 94720-7450, USA
Institute for Physical Science and Technology, University of Maryland, College Park, MD 20742, USA
Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, California, USA
University of California, San Diego, La Jolla, CA, US
Space Sciences Laboratory, Berkeley, CA, USA;
University of California, San Diego, CA, US
University of California, La Jolla, CA, US
Space Sciences Laboratory, University of California, Berkeley, California, USA
Space Science Laboratory, UCB, Berkeley, CA, USA
Maryland, University, College Park
Space Sciences Laboratory, UC Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450, USA
University of California, San Diego, LaJolla, CA, US
SciberQuest, Inc., Solana Beach, CA, 92075
ECE Department, UCSD, 9500 Gilman Drive, La Jolla, CA 92093-0407, USA University of California, Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California - Berkeley, 7 Gauss Way, Berkeley, CA 90095, USA
UCSD, ECE Department, 9500 Gilman Drive, La Jolla, CA 92093-0407, USA Univ., La Jolla
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA
Space Sciences Laboratory, UCB, 7 Gauss Way, Berkeley, CA 94720-7450, USA
University of California, Berkeley, Space Sciences Laboratory, MC 7450 7 Gauss Way, Berkeley, CA 94720-7450, USA
Space Sciences Laboratory, MC 7450 7 Gauss Way University of California, Berkeley, ca 94720-7450, USA
Space Sciences Laboratory, UC Berke
A mirror instability associated with newly created ions in a moving plasma
A New Simulation Technique for Study of Collisionless Shocks: Self-Adaptive Simulations
A test of the Hall-MHD model: Application to low-frequency upstream waves at Venus
Alfven/Ion-Cyclotron Waves Observed on the Earthward Side of a Solar Wind Reconnection Exhaust?
Asymmetric shear flow effects on magnetic field configuration within oppositely directed solar wind reconnection exhausts
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