Simulation of the Cosmic Ray Moon Shadow in the Geomagnetic field

Details Simulation of the Cosmic Ray Moon Shadow in the Geomagnetic field Simulation of the Cosmic Ray Moon Shadow in the Geomagnetic field

2009-07-07

arxiv.org/abs/0907.1173v1

Nucl.Instrum.Meth.A630:301-305,2011

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

4 pages, 5 figures, Contribution to the 31st ICRC, Lodz, Poland, July 2009

Scientific paper

10.1016/j.nima.2010.06.197

An accurate MonteCarlo simulation of the deficit of primary cosmic rays in the direction of the Moon has been developed to interpret the observations reported in the TeV energy region until now. Primary particles are propagated trough the geomagnetic field in the Earth-Moon system. The algorithm is described and the contributions of the detector resolution and of the geomagnetic field are disentangled.

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