Slide 1 Today: How a star changes while on the main sequence What happens when stars run out of hydrogen fuel Second stage of thermonuclear fusion Star clusters and stellar…
1 RVCQ3D - Rotor Viscous Code Quasi-3-D User’s Manual and Documentation Version 303, March 1, 1999 Dr. Rodrick V. Chima NASA Glenn Research Center, MS 5-10 21000 Brookpark…
A Long-term Sunspot Magnetic Field Decrease William Livingston (NSO) Rachel MacDonald (Yale) Tom Schad (UAz) Space Weather Workshop Intro to spectra Dark umbral cores observed…