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Documents Today: How a star changes while on the main sequence What happens when stars run out of hydrogen...

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…

Documents fluid flow Q3D

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…

Documents A Long-term Sunspot Magnetic Field Decrease

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…