Physics
Scientist
CUA and NASA / GSFC
Code 682, Solar Physics Branch, Laboratory for Astronomy and Solar Physics, NASA / Goddard Space Flight Center, Greenbelt, Maryland 20771 and Department of Physics, The Catholic University of America, Washington, DC 20064
Code 682, Solar Physics Branch, NASA / Goddard Space Flight Center, Greenbelt Maryland 20771, and Department of Physics, The Catholic University of America, Washington, DC 20064
MIT, Cambridge, MA
Code 682, Solar Physics Branch, Laboratory for Astronomy and Solar Physics, NASA / Goddard Space Flight Center, Greenbelt, Maryland 20771 and Department of Physics, The Catholic University of America, Washington, D.C. 20064
Lab for Astr. and Solar Phys., NASA / Goddard
NASA, Goddard Space Flight Center, Greenbelt, MD
The Catholic University of America, Department of Physics, 200 Hannan Hall, 620 Michigan Ave., Washington, District of Columbia 20064; NASA / GSFC, Code 682, Greenbelt, Maryland 20771
A Balloon-Borne Payload for Imaging Hard X-Rays and Gamma-Rays from Solar Flares
An Optical Method for Quantitatively Characterizing Rotating Modulation Collimators (RMC)
Cross sections for production of the 15.10 MeV and other astrophysically significant gamma-ray lines through excitation and spallation of12 C and16 O with protons
Cross Sections for Production of the 15.10-MeV and Other Astrophysically Significant Gamma-Ray Lines
Cross sections for production of the 15.10-MeV and other astrophysically significant gamma-ray lines through excitation and spallation of 12C and 16O with protons
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