Difference between revisions of "HRRL RS"
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[[Roman calculation]] | [[Roman calculation]] | ||
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| + | Ðîìà! | ||
| + | Ñîäåðæèìîå äèñêà ðàçáèòî íà 3 àðõèâà. Ïðàâäà ñíà÷àëî ïðèøëîñü óäàëèòü âåñü îôèñ, íî åãî ïîòîì ÿ òîæå äîáàâèë-ôàéë rom_add(2÷àñòè). | ||
| + | ×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). | ||
| + | Ïîñëåäíþþ ÷àñòü àðõèâà âîçüìè íà oyb13 ïàðîëü tooper1 | ||
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[[optical coupling compound]] | [[optical coupling compound]] | ||
Revision as of 03:50, 19 February 2012
PhotoFission with Polarized Photons from HRRL
anisotropic n's vs. isotropic ones
some notes about shielding materials
2n correlations in Photofission
Ðîìà! Ñîäåðæèìîå äèñêà ðàçáèòî íà 3 àðõèâà. Ïðàâäà ñíà÷àëî ïðèøëîñü óäàëèòü âåñü îôèñ, íî åãî ïîòîì ÿ òîæå äîáàâèë-ôàéë rom_add(2÷àñòè). ×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). Ïîñëåäíþþ ÷àñòü àðõèâà âîçüìè íà oyb13 ïàðîëü tooper1