Angle-Time-Energy Images of Ultra-High Energy Cosmic Ray Sources
arXiv:astro-ph/9712144 · doi:10.1063/1.56142
Abstract
Substantial amount of information both on the source and on characteristics of intercepting magnetic fields is encoded in the distribution in arrival times, directions, and energies of charged ultra-high energy cosmic rays from discrete sources. We present a numerical approach that allows to extract such information from data from next generation experiments.
9 latex pages, 3 postscript figures included, uses (and includes) aipproc.sty and epsfig.sty. To appear in Proceedings of the Workshop on "Observing Giant Cosmic Ray Air Showers for > 10**(20) eV Particles from Space", Univ. of Maryland, Nov 13-15, 1997. Summary version of astro-ph/9711060