Physics
Scientist
University of Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA University of Washington, Geophys Program, Seattle, WA 98195 USA Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA University of Iowa, Department Phys & Astron, Iowa City, IA 52242 USA
Space Sciences Laboratory, University of California, Berkeley, California, USA
California, University, Berkeley, Calif.
Physics Department and Space Sciences Laboratory, University of California, Berkeley, California 94720
University of California, Berkeley, CA, US
Space Sciences Laboratory, University of California, Berkeley, CA, USA
California, University, Berkeley, CA
California Univ., Berkeley.
Berkeley, California, USA
University of California Space Sciences Lab Berkeley, CA 94720, USA
Space Sciences Lab UC Berkeley, 1062 Woodside Rd., Berkeley, CA 94708, USA Sciences Lab, University of California-Berkeley, 7 Gauss Way, Berkeley, CA 94720-7450, USA of California, Berkeley, Space Sciences Lab 7 Gauss Way, Berkeley, CA 94720-7450, USA
California, University, Berkeley
SSL / University of California, Space Sciences Lab, Berkeley, CA 94720, USA Science Laboratory, University of California, Berkeley CA 94720-7450, USA
California Univ., Berkeley
Space Sciences Laboratory, University of California at Berkeley, CA 94720, USA
Space Sciences Laboratory, University of California, Berkeley, Berkeley, California 94720
Space Sciences Laboratory, 7 Gauss Way, Berkeley, CA 94720-7450
Space Sciences Laboratory, University of California, Berkeley, Berkeley, California, USA
Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA / University of California, University of California, Berkeley, CA 94720, USA
A comment on the source region of VLF saucers
A new model for the prediction of Dst on the basis of the solar wind
A radial diffusion simulation of energetic particles in ULF compressional fluctuations
A Real-time Forecast Model for the Dst Index
Aircraft observations conjugate to FAST: Auroral arc thicknesses
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