Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
NASA, Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, MD
NASA, Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt; Applied Research Corp., Landover, MD
NASA, Goddard Space Flight Center, Greenbelt, MD
National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, MD.
NASA Goddard Space Flight Center, Lab for Solar and Space Physics, Code 612.1, Greenbelt, MD 20771, USA Goddard Space Flight Center, Code 612.1, Greenbelt, MD 20771, USA Goddard Space Flight Center, Lab for Solar and Space Physics, code 612.1, Greenbelt, MD 20771, USA / GSFC
NASA / Goddard Space Flight Center
NASA-GSFC, Code 671.0, Greenbelt, MD 20771, USA
Solar Physics Branch, Code 682, Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Laboratory for Astronomy and Solar Physics, Code 682.2, NASA / GSFC, Greenbelt, MD 20771, USA
Code 682, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
Code 682, NASA Goddard Space Flight Center, Greenbelt, MD 20771
Goddard Space Flight Center, NASA, Greenbelt, MD, USA; Physics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA; Laboratory, Hanscom
NASA Goddard Space Flight Center, Greenbelt, MD 20771 Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, Md.
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Goddard Space Flight Center, Greenbelt, MD, US
NASA-GSFC
NASA's GSFC
National Aeronautics and Space Administration. Marshall Space Flight Center, Huntsville, AL.
ST Systems Corp., Lanham, MD.
National Aeronautics and Space Administration. Goddard Spac
25-250 keV X-Ray Observations of Cygnus XR-1
A 2.2 second period in the 1984 August 5 gamma-ray burst
A Balloon-Borne Payload for Imaging Hard X-Rays and Gamma-Rays from Solar Flares
A Comparison of Pulse Trains in the Solar Hard X-ray Flares of 1980 June 7 and 1983 May 12
A correlation between 4-8 MeV gamma-ray-line fluence and >~50 keV X-ray fluence in large solar flares
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