Difference between revisions of "File:HuntsIACgraphs.pdf"

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-When I got boared one day on vacation I started going through the prompt
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-gamma-ray data that we have.  Found something a little bit interesting
-with regards to the times that the asymetric peaks arrive.  They appear
-to be much more spread out in time.  Anyway I attach a PDF with 6
-figures and hopefully a somewhat coherent description of the figures.
-  I also attach the Origin file incase you want to zoom around the figures
-or play with anything.
-  Also the dominant peaks without coincedence at 388 and 333 keV, I think
-those are from Cf-249, which has a half life of a few 351 years.  I am
-not sure if it is a contaminant when they make the source or if it grows
-in over time.  When Cf-252 alpha decays it becomes Cm-249, which beta-
-decays to Bk-249.  Bk-249 then beta- decays again to Cf-249.Cf 249 also
-has a little line at 252.8 keV, which is also in the spectrum.  So I
-think those dominant lines are from Cf-249.