- Solar and Stellar Atmospheres
- Supernovas & Remnants
- Atomic & Molecular Data
- Black Holes
- Interstellar Medium and Molecular Clouds
John Raymond applies spectroscopy and plasma physics in an attempt to understand the the heating of the solar corona, the driving of the solar wind, the nature of supernova remnant shock waves, sungrazing comets and the winds from black hole accretion disks.
PhD, University of Wisconsin