Email: jhamilton58 at gsu dot edu
I am currently attending Georgia State University as a Ph.D. student. My background thus far spans structure and evolution of low mass stars with starspots, evolution of globular clusters with varied abundances for multiple populations, to red giants in binary pairs for asteroseismic analysis. Currently, I am working with the solar physics team under Dr. Viacheslav Sadykov modeling radiative transfer in the solar atmosphere to understand the morphology of spectral lines due to wave propagation and the correlation to the flow of energy.