Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
NASA, Goddard Space Flight Center, Laboratory for Extraterrestrial Physics, Greenbelt, MD
National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, MD.
NASA, Goddard Space Flight Center, Laboratory for Extraterrestrial Physics, Greenbelt, Space Flight Center, Greenbelt, Greenbelt, MD 20771, USA Goddard Space Flight Center, Code 612 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Goddard Space Flight Center, Greenbelt, Maryland, USA
NASA, Goddard Space Flight Center, Greenbelt, Md.
NASA / GSFC, Laboratory for Solar and Space Physics, NASA / GSFC, Code 612.3, Greenbelt, MD 20771, USA Goddard Space Flight Center
Laboratory for Solar and Space Physics, NASA / GSFC, Code 612.3 NASA / GSFC, Greenbelt, MD 20771, USA / Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
Laboratory for Solar and Space Physics, NASA / Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
NASA, Goddard Space Flight Center, Greenbelt, MD
Laboratory for Extraterrestrial Physics, NASA-Goddard Space Flight Center, Greenbelt, MD 20771, USA
Goddard Space Flight Center, NASA, Greenbelt, MD, USA
Space Weather Laboratory, GSFC / NASA, Greenbelt, Maryland, USA
Space Weather Laboratory, NASA / GSFC
Laboratory for Extraterrestrial Physics NASA-Goddard Space Flight Center
Heliophysics Science Division, NASA / GSFC
Space Science Center, University of New Hampshire, NH, USA
Space Science Center, University of New Hampshire, Durham, NH, USA
Catholic University of Am.
NASA / Goddard Space Flight Center, Code 696, Greenbelt, MD 20771, USA
A comparative review of bow shocks and magnetopauses
A comparative study of Solar-Heliospheric Observations during very active Sun intervals in the 21st and 23rd solar cycles (April 1979 and March-April, 2001)
A comparison of a model for the theta aurora with observations from Polar, Wind, and SuperDARN
A Correlative Study of SSC's, Interplanetary Shocks, and Solar Activity
A high time resolution study of the solar wind-magnetosphere energy coupling function
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