+ Hard X-Ray Footpoint Motion and Progressive Hardening in Solar Flares Margot Robinson Mentor: Dr. Angela DesJardins MSU Solar Physics Summer REU, 2010.
Best-fit Power laws ( A D z B + C ): V SW : A = 1.49 (± 0.19) 10 -5 B = 4.56 ± 0.33 (1)
