Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Laboratory for Astronomy and Solar Physics, Code 612.1, NASA Goddard Space Flight Center, Greenbelt, MD 20771; Department of Physics, Catholic University of America, 620 Michigan Avenue NE, Washington, DC 20064
Laboratory for Astronomy and Solar Physics, Code 682, NASA Goddard Space Flight Center, Greenbelt, MD 20771; Department of Physics, Catholic University of America, 620 Michigan Avenue, Washington, DC 20064. for Astronomy and Solar Physics, Code 682, NASA Goddard Space Flight Center, Greenbelt, MD 20771; Also at: Department of Physics, Catholic University of America, 620 Michigan Avenue, Washington, DC 20064.
Department of Physics, Catholic University of America, Washington, DC 20064; Laboratory for Solar and Space Physics, Code 612.1, NASA Goddard Space Flight Center, Greenbelt, MD 20771.
The Catholic University of America, District of Columbia, USA
NASA / GSFC & CUA
CUA & Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
CUA / NASA's GSFC
Department of Physics, Catholic University of America, Washington, DC 20064; NASA Goddard Space Flight Center, Solar Physics Laboratory, Code 671, Greenbelt, MD 20771.
Catholic University of America, Department of Physics, 200 Hannan Hall, 620 Michigan Ave, Washington, DC 20064, USA; 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; The Catholic University of America, 620 Michigan Avenue, N. E., Washington, DC 20064, USA University of America, Department of Physics, 200 Hannan Hall, Washington, DC 20064, USA; NASA Goddard Space Flight Center, Lab for Solar and Space Physics, code 612.1, Greenbelt, MD 20771, USA / GSFC
Catholic University of America; NASA God
A Multi-wavelength Analysis of a Solar Limb Flare on 2002 April 15
A Statistical Analysis of Loop-Top Motion in Solar Limb Flares
Determination of Low-Energy Cutoffs and Total Energy of Nonthermal Electrons in a Solar Flare on 2002 April 15
Direct observation of high-speed plasma outflows produced by magnetic reconnection in solar impulsive events
Direct Observation Of High-speed Plasma Outflows Produced By Magnetic ReconnectionIn Solar Impulsive Events
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