ÂÜÀòÂÒÂ×

Sarah Bruce is a Graduate Research Hale Fellow at the National Solar Observatory, currently designing and launching an instrument to measure K-Coronal temperatures. Prior experience includes being an Undergraduate Researcher at The University of Texas at Austin in Galaxy Evolution and Experimental Geometry projects. Additionally, Sarah has worked as a Solar Physics Research Intern at the Center for Astrophysics | Harvard & Smithsonian. Sarah holds a Bachelor of Science in Mathematics from The University of Texas at Austin and is currently pursuing a Doctor of Philosophy in Astrophysics at the University of Colorado Boulder.