'Cosmic ray energies' presentation slideshows

Chapters 7,8: Formation of the Solar System

Chapters 7,8: Formation of the Solar System. Stars, solar systems form within giant molecular clouds Requires high density , dust, and low temperatures to initiate gravitational collapse

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1927-28 Jacob Clay from Genoa to the Dutch colony of Java

687 views • 54 slides

1927-28 Jacob Clay from Genoa to the Dutch colony of Java

567 views • 54 slides

Search for EHE neutrinos with the IceCube detector

Search for EHE neutrinos with the IceCube detector. Aya Ishihara for the IceCube collaboration Chiba University. atmospheric muon flux above 10 6 GeV is very uncertain. EHE Neutrino Underground. Surface n fluxes. Target GZK neutrino Surface energy range 8 < Log(E/GeV) < 12

264 views • 17 slides