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Cosmic Ray Anisotropy Workshop 2017

9–14 Oct 2017
Guadalajara, Mexico
Mexico/General timezone

Session

Session IX

9
12 Oct 2017, 14:05
Guadalajara, Mexico

Guadalajara, Mexico

Hotel Krystal Urban Guadalajara Av. López Cotilla No. 2077 Col. Arcos Vallarta Guadalajara, Jalisco, 44130

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  1. 3. Heliospheric Tail Models
    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...
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  2. 46. Heliospheric modulations
    Prof. Ming Zhang (Florida Institute of Technology)
    12/10/2017, 14:50
  3. 44. Numerical Modeling
    12/10/2017, 15:25
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