Constrained Simulations of the Magnetic Field in the Local Supercluster and the Propagation of UHECR

Details Constrained Simulations of the Magnetic Field in the Local Supercluster and the Propagation of UHECR Constrained Simulations of the Magnetic Field in the Local Supercluster and the Propagation of UHECR

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....2..735d&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

Magnetic fields (MF) in the local supercluster (LSC) of galaxies may have profound consequences for the propagation of Ultra High Energy Cosmic Rays (UHECR). Faraday rotations measurements provide some informations about MF in compact clusters. However, very few is known about less dense regions and about the global structure of MF in the LSC. In order to get a better knowledge of these fields we are performing constrained magnetohydro dynamical simulations of the LSC magnetic field. We will present the results of our simulation and discuss their implications for the angular distribution of expected UHECR deflections.

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