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Scientist
Physics Department, University of Connecticut, Storrs, CT 06269; Institute of Materials Science, University of Connecticut, Storrs, CT 06269
Contributors to the solar-wind-induced spectrum of cometary x-rays: S and Ne L x-rays, Fe M x-rays and others
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 and Optical Laboratory Spectra to Simulate the Solar Wind on Comets: O5+ + CO
Soft X-ray Line Emission Spectra from Highly-Charged Solar Wind Ions on Cometary Gases: N^5,6+ on CO
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