Physics
Scientist
University of Connecticut
Relative XUV/soft x-ray emission cross sections for charge transfer from cometary gases to O^q+ in the 10 -50 KeV range.
Simulation of cometary x rays in collisions of keV C^5+, C^6+, Ne^8+ with CO, H2, and He
Soft X-ray Line Emission Spectra from Highly-Charged Solar Wind Ions on Cometary Gases: N^5,6+ on CO
Visible spectroscopy of collisions of solar-wind ions on gas targets of astrophysical interest
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