Cascades initiated by EHE photons in the magnetic field of the Earth and the Sun
W. Bednarek (Department of Experimental Physics, University of Lodz,, Poland)

TL;DR
This paper uses Monte Carlo simulations to analyze how extremely high energy photons interact with Earth's and Sun's magnetic fields, predicting cascade probabilities and identifying unique observational signatures for these rare cosmic events.
Contribution
It introduces a detailed simulation framework for EHE photon cascades in Earth's and Sun's magnetic fields, highlighting directional dependencies and potential observational markers.
Findings
Higher cascade probability from magnetic poles.
Lower cascade probability from equatorial directions.
Potential detection of unusual showers from the Sun's magnetosphere.
Abstract
The content of extremely high energy (EHE) photons in the highest energy cosmic rays can be investigated by analyzing showers arriving from directions where the perpendicular component of the Earth's magnetic field is high or showers arriving from the region surrounding the Sun. We perform Monte Carlo simulations of cascades initiated by photons with parameters of the highest energy showers observed by the past and present detectors (AGASA, Fly's Eye, Yakutsk, Haverah Park). The purpose is to find out which events should cascade with high probability if initiated by photons. It is shown that EHE photons arriving from directions towards the magnetic poles cascade with higher probability. Alternatively, the lowest probabilities of cascading are expected for photons arriving from directions of the equator at the zenith angles equal to the angle between location of the specific observatory…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics
