July 16 - 20

We were able to do a Guassian fitting for the acceleration profiles to calculate the peak acceleration and duration (full width at half maximum) for each event. I spent most of the week cleaning up/making smooth JMAPs across all three field of views (each JMAP contains the three field of views of STEREO that goes out to 15 solar radii) for as many events I could. The biggest problem I ran into was that sometimes there'd be no definition of the front in the EUVI field of view (where most acceleration occurs of a CME). I've attached an example of the new Guassian fitting: