Physics
Scientist
Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA Hopkins University Applied Physics Laboratory, Mailstop MP3-W189 11100 Johns Hopkins Road, Laurel, MD 20723, USA Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA Hopkins University Applied Physics Laboratory, Mailstop MP3-W189, 11100 Johns Hopkins Road, Laurel, MD 20723, USA
Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA
Hanscom
Johns Hopkins University, Laurel, MD
Johns Hopkins University, Laurel, MD, US
ECE, Virginia Tech, Blacksburg, VA, USA; Dept. of Electrical and Computer Engineering, Virginia Tech, Blacksburg, VA, USA; Physics Laboratory, Johns Hopkins University, Laurel, Maryland, USA
Massachusetts Institute of Technology, Haystack Observatory, Westford, MA, USA, USArecibo Observatory, Arecibo, Puerto Rico, PRCalifornia Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA, USA, USThe John Hopkins University, Applied Physics Laboratory, Laurel, MD, USA, USArecibo Observatory, Arecibo, Puerto Rico, PRCornell University, School of Electrical Engineering, Ithaca, NY, USA, USSRI International, Geoscience and Engineering Center, MenloPark, CA, USA, USCalifornia Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA, USA, US
Johns Hopkins University, Applied Physics Laboratory, 11100 Johns Hopkins Rd, Laurel, MD 20723-6099, USA
Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099, USA Johns Hopkins University Applied Physics Lab, Laurel, MD, US
Johns Hopkins Univ., Laurel, MD
Virginia Polytechnic and State University, 302 Whittemore Hall, Blacksburg, VA 24061, USA Polytechnic Institute and State Universit
A case study of relationship between substorm expansion and global plasma convection
A new method for detecting the projection of magnetospheric oscillations into the ionosphere
A New Statistical Convection Model Derived from SuperDARN and Polar UVI Observations
A New Statistical Convection Model Derived from SuperDARN and Polar UVI Observations
A possible explanation for rapid, large-scale ionospheric responses to southward turnings of the IMF
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