July 23-27

Given the new Guassian fitting, I went back and further cleaned-up the JMAPs to get nice Guassians in preparation for reconnection data comparison. Since Chunming leaves for Florida next week, I presented at our weekly Solar meeting and showed off two histograms, one showing the distribution of events' max accelerations and the other showing the distribution of durations (full width at half max) of the CMEs. I've attached these histograms below: