Physics
Scientist
NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
NASA's Goddard Space Flight Center, Laboratory for Solar and Space Physics, Greenbelt, MD 20771, USA Goddard Space Flight, Heliospheric Physics Branch Mail Code 612.2 Building 21, Room 254A, Greenbelt, MD 20771, USA
NASA Goddard Space Flight Center, Heliospheric Physics Branch Mail Code 612.2 Building 21, Room 254A, Greenbelt, MD 20771-1000, USA
NASA Goddard Space Flight Center, Laboratory for Solar and Space Physics, 8800 Greenbelt Road, Greenbelt, MD 20770, USA
NASA / Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA
NASA / Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD 20771-1000, USA
Geospace Science Laboratory, Code 673 NASA Goddard Space Fight Center, Greenbelt, MD 20771, USA for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35899, USA Marshall Space Flight Center, Huntsville, AL
Alabama University
NASA / Marshall Spaceflight Center, NSSTC, SD50, Huntsville, AL 35899, USA Space Science and Technology Center, NASA / Marshall Space Flight Center, Mail Code SD50, Huntsville, AL 35812, USA Space Science and Technology Center, NASA Marshall Space Flight Center / SD50, Huntsville, AL 35812, USA Space Science and Technology Center / NRC, 320 Sparkman Dr, Huntsville, AL 35805, USA / Marshall Space Flight Center, National Space Science and Technology Center, Space Science Department, SD-50, 320 Sparkman Drive, Huntsville, AL 35805, USA Physics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
NASA Goddard Space Flight Center, Heliophysics Sci
Bursty Electromagnetic Waves Associated with Turbulent Magnetic Reconnection
Bursty, Broadband Electromagnetic Waves Associated with Thin Current Layers and Turbulent Magnetosheath Reconnection
Cluster observations of EMIC triggered emissions in association with Pc1 waves near Earth's plasmapause
Compositional Variability of the Solar Wind: The Need for an Ultra-High Temporal Resolution Mass Spectrometer for Studies of Solar Wind and Coronal Mass Ejection Boundaries
Determining the dynamic range of MCPs based on pore size and strip current
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