Physics – Geophysics
Scientist
Physics
Geophysics
Scientist
Department of Electrical Engineering, Stanford University, Stanford, California, USA
Stanford University, Packard Building Room 315, 350 Serra Mall, Stanford, CA 94306-9515, USA
Stanford University, 350 Serra Mall, Stanford, CA 94305, USA Telecommunications, and Radioscience Laboratory, Stanford University, Stanford, California, USA
STAR Laboratory, Department of Electrical Engineering, Stanford University, Stanford, California, USA
Electrical Engineering Department, Stanford University, Stanford, California, USA
Electrical Engineering, Stanford University, Stanford, CA, USA;
Department of Electrical Engineering, Stanford University, Stanford, CA, USA;
STAR Lab, Stanford University, 350 Serra Mall, Stanford, CA 94305-9515, USA University, Packard Bldg Rm 315 350 Serra Mall, Stanford, CA 94306, USA Lab, Stanford University, Stanford, CA 94305, USA
Stanford University, Packard Bldg Rm 321 350 Serra Mall, Stanford, CA 94305, USA
STAR Laboratory, Electrical Engineering Department, Stanford University, Stanford, California, USA
Space Science Laboratory, University of California, Berkeley, CA 94720, USA Telecommunications, and Radioscience Laboratory, Department of Electrical Engineering, Stanford University, Stanford, California, USA
STAR Laboratory, Stanford University, Stanford, CA 94305, USA
Stanford University, STAR Lab, 350 Serra Mall, Stanford, CA 94305, USA University, STAR Lab, 350 Serra Mall, Stanford, CA 94305-9515, USA
Stanford University, Packard Bldg Rm 351, Stanford, CA 94305, USA University, Electrical Engineering, Stanford University, Stanford, CA 94305, USA of California, Berkeley, Space Sciences Lab, Berkeley, CA 94720, USA Lab, Department of Electrical Engineering, S
Afternoon Subauroral Proton Precipitation Resulting from Ring Current - Plasmasphere Interaction
Antarctic Ground-based Observations During Selected THEMIS Satellite Event Studies
Antarctic Observations of Dayside Auroral Hiss
Calculating Wave Power from the Source Particle Distributions for EMIC Waves
Comparison of chorus wave power during CIR versus CME-driven geomagnetic storms
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