Dr
Klaus Scherer
(Ruhr University Bochum)
12/10/2017, 14:05
Invited Talk
In the tail direction of the heliosphere an anisotropy in the cosmic
ray flux is observed by the large area telescopes. These ansiotropy is
partly explained by the modulation of cosmic rays in the tail
region. But, most of the modeling of the large scale heliosphere is
concentrated on the nose direction, because there are the in situ
observations of the Voayger spacecraft available. The...
