Simulation of the Cosmic Ray Moon Shadow in the Geomagnetic field
classification
🌌 astro-ph.HE
keywords
fieldgeomagneticcosmicmoonprimarysimulationaccuratealgorithm
read the original abstract
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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.