Computer Science – Data Structures and Algorithms
Scientist
Computer Science
Data Structures and Algorithms
Scientist
Sandia National Laboratories
IGPP, 3845 Slichter Hall, Los Angeles, CA 90095
UCLA, IGPP, UCLA, Los Angeles, CA 90024, USA
University of California, Los Angeles, Institute of Geophysics and Planetary Physics, Los Angeles, CA 90095-1567, USA of California, Los Angeles, Institute of Geophysics, Los Angeles, CA 90095, USA of Delaware
Institute of Geophysics and Planetary Physics, 405 Hilgard Ave., Los Angeles, CA 91411, USA of Geophysics and Planetary Physics, University of California, 405 Hilgard Ave, Los Angeles, CA 90095-156, USA of Geophysics, University of California, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA, USA
IGPP, box 951567 UCLA, Los Angeles, ca 90095, USA of Geophysics and Planetary Physics, University of California, 3845 Slichter Hall, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA 90095, USA
IGPP / UCLA, IGPP / ESS Univercity of California, Los Angeles, CA 90095, USA / UCLA, Box 951567, Los Angeles, CA 90095, USA
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA
IGPP UCLA, 405 Hilgard Ave, Los Angeles, CA 90095, USA
IGPP / UCLA, 405 Hilgard Ave, Los Angeles, c 90095, USA of Geophysics and Planetary Physics, University of California, Los Angeles, Los Angeles, CA 90095, USA
University of California Los Angeles
Universtiy of California at Los Angeles, Institute of Geophysics 405 Hilgard Ave, Los Angeles, CA 90095, USA
IGPP, University of California, Los Angeles, CA 90095, USA
Institute of Geophysics and
1D Hybrid Simulations of Ion Cyclotron Wave Generation by Pickup Ions at Titan
3D Modeling of the Massive Binary Wind Interaction Region in Eta Carinae
3D Reconstruction of the 22 May 2007 Magnetic Cloud: How Much Can We Trust the Flux- Rope Geometry of CMEs?
A Comparison of Cluster Observations of the Tail Current during Substorms and Quiet Times
A Preliminary Comparison Between SuperDARN Flow Vectors and Equivalent Ionospheric Currents From the GIMA, Greenland, MACCS, THEMIS, CARISMA, and CANMOS Ground Magnetometer Arrays
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