WEEK FIVE
















June 29,2009

I was able to move to a different computer to verify that the xwin programs was the problem with the OSPEX GUI but the problem is in the OSPEX problem. Now the next step is to contact Kim the writer of the OSPEX GUI.



I started to look at Amanda Dillman's, a REU student from 2005, plotting programs to make graphs of the various components with respect to time.








June 30, 2009



Made RHESSI overlays using a different mdi magnetogram.










Impulsive phase
1:42:05- 2:00:53





Time start- 1:54:40
Time end- 1:55:00













Time Start- 1:57:40
Time End-1:58:30












Time Start-1:58:30
Time End-1:59:40












Time Start- 1:59:40
Time End-2:00:53










Peak

Time Start- 2:00:50
Time End-2:02:00











DECAY PHASE

Time Start- 2:03:07
Time End-2:06:00











July 1, 2009



I started writing a program to correct the pointing on the TRACE with reference to the SOHO MDI information for my flare. The TRACE files for my flare finished downloading in the late afternoon and I started working on a movie. TRACE is the Transition Region and Coronal Explorer its  a NASA Small Explorer mission to take images of the solar corona at high angular and temporal resolution. For more information check out the official TRACE web site.



                                    
                                             
   FLARE X 1 MOVIE
                                            







July 2, 2009



I realized the program I was writing would not  help me due to the TRACE files I have are all corrected. All I need to use is one program called trace_mdi_align. Unfortunately once I input both fits files for SOHO MDI and TRACE into the program its output told me it could not find "GET ORBIT" data so now I have to figure out where it might me located in the structure.

Brian Dennis, an Astrophysicist from Goddard, told Angela about a new program called HSI_SPECTRUM_SEP_DET_FILES. Its purpose is to generate separated spectrum and srm files for each RHESSI detector when given the time interval of the flare. This is a new way to analyze spectral data. The spectrum plots for each detector are below.



Detector 1




Detector 2




Detector 3






Detector 4




Detector 5






Detector 6





Detector 7





Detector 8





Detector 9