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Dr Jens Kleimann (Ruhr-Universität Bochum)12/10/2017, 16:30Invited TalkStudying the propagation of charged cosmic rays requires a realistic prescription of the background magnetic field of the traversed environment, such as the Galaxy or the heliosphere. In the latter case, analytic models may provide a less accurate, yet simpler and more accessible alternative to computationally expensive high-resolution magnetofluid simulations. In this talk, I will present and...Go to contribution page
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Dr Klaus Scherer (Ruhr University Bochum)12/10/2017, 17:05Invited TalkLarge area telescope show spatial anisotropies of the high energy cosmic ray flux in the permille. We model the cosmic ray flux through a sphere of 1 kpc, in which we have located different astrosphere (or the like) with a radii varying from 1 to 10\,pc at a large distance from the observer. We discuss cosmic ray anisotropies for different setups of the location of the astrospheres. We...Go to contribution page
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