... Loss direction to origin in the Galactic magneticfield (~10 G or 1nT, thickness 200-300pc) For 100TeV proton: "9 ! ... Local Interstellar MagneticField + Heliosphere (argued because heliosphere can't inf luence CRs >10TeV, but anisotropy obser ...
[
Текст
]
Ссылки http://antares.sinp.msu.ru/docs/Anisotropy_2011Bamberg.pdf -- 1353.8 Кб -- 16.12.2013 Похожие документы