Computer Science – Sound
Scientist
Computer Science
Sound
Scientist
Lockheed Space Sciences Laboratory, Palo Alto, CA
LASP, University of Colorado, Boulder, CO, USA
Laboratory of Atmospheric and Space Physics, University of Colorado, 1234 Innovation Drive, Boulder, CO 80304, USA
Johns Hopkins University, Baltimore, Md.
University of Colorado - LASP, 1234 Innovation Dr, Boulder, CO 80303, USA
University of Colorado, LASP, 1234 Innovation Dr., Boulder, CO 80303, USA for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado, USA
Lockheed Research Laboratories, Palo Alto, CA
Space Science Lab., Palo Alto, CA, US
Lockheed Martin, Advanced Technology Center, Palo Alto, CA 94304, USA
LASP, University of Colorado, Boulder, CO, USA;
Physics and Astronomy, George Mason university, Fairfax, VA, USA;
School of Physics and Astronomy, 116 Church St. SE, University of Minnesota, Minneapolis, MN 55455 USA
Lockheed Missiles and Space Laboratories, Palo Alto, Calif.
University of Colorado, LASP, Boulder, CO 80303, USA of Atmospheric and Space Physics, University of Colorado, Boulder, CO 80309-0392, USA
Phillips Laboratory, Hanscom
Lockheed Missiles and Space Co., Inc., Palo Alto, CA
Lockheed Research Laboratory, Palo Alto, CA
Lockheed Space Science Laboratory, Palo Alto, CA
Lockheed Martin Palo Alto Research Laboratory, 0 / H1-11, B / 252, 3251 Hanover St Palo Alto, CA 94304, USA
LASP, University of Colorado, Boulder, CO 80309-0392, USA University of Colorado, Boulder, Colorado, USA
Lockheed Martin Advanced Technology Center, 3251 Hanover St., Palo Alto, CA 94304, USA
Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA
Lockheed Space Sciences L
<formula alphabet="latin">O+ observations in the cusp: Implications for dayside magnetic field topology
A comparison of a model for the theta aurora with observations from Polar, Wind, and SuperDARN
A global comparison of O+ upward flows at 850 km and outflow rates at 6000 km during nonstorm times
A global view of O+ upwelling and outflow rates between DMSP and POLAR
A simple model of complex cusp ion dispersions during intervals of northward interplanetary magnetic field
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