Difference between revisions of "HRRL RS"

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Ðîìà!
 
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Ñîäåðæèìîå äèñêà ðàçáèòî íà 3 àðõèâà. Ïðàâäà ñíà÷àëî ïðèøëîñü óäàëèòü âåñü îôèñ, íî åãî ïîòîì ÿ òîæå äîáàâèë-ôàéë rom_add(2÷àñòè).
 
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×òîáû äèñê áûë ïîëíûì, íóæíî ñíà÷àëà ðàçàðõèâèðîâàòü 3 ÷àñòè, à ïîòîì äîïîëíèòåëüíûå ðàçàðõèâèðîâàòü è  ïîëîæèòü â íóæíóþ ïàïêó.(åå ÿ àðõèâèðóþ ñ ïðàâèëüíûì ïóòåì).
 
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Ïîñëåäíþþ ÷àñòü àðõèâà âîçüìè íà oyb13 ïàðîëü tooper1
 
  
  

Revision as of 03:51, 19 February 2012

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PhotoFission with Polarized Photons from HRRL


plan to do 04/11/2011

n's detector calibration

photo-nuclear sigma

anisotropic n's vs. isotropic ones

some notes about shielding materials

2n correlations in Photofission

Roman calculation




optical coupling compound

Retrieved from "https://wiki.iac.isu.edu/index.php?title=HRRL_RS&oldid=71385"