Density and magnetic intensity dependence of radio pulses induced by energetic air showers
Juan Ammerman-Yebra, Jaime Alvarez-Mu\~niz, Enrique Zas

TL;DR
This study extends a simulation program to analyze how atmospheric density and magnetic field strength influence radio pulses from energetic air showers, revealing complex scaling behaviors and spectral properties.
Contribution
It introduces a magnetic field extension to the ZHS simulation, enabling realistic modeling of radio pulses in atmospheric conditions with variable density and magnetic field.
Findings
Electric field amplitude scales non-linearly with magnetic field strength.
A precise scaling law relates pulse spectra across different densities and magnetic fields.
Spectral behavior is explained in terms of shower development parameters.
Abstract
We have studied the effect of changing the density and magnetic field strength in the coherent pulses that are emitted as energetic showers develop in the atmosphere. For this purpose we have developed an extension of ZHS, a program to calculate coherent radio pulses from electromagnetic showers in homogeneous media, to account for the Lorentz force due to a magnetic field. This makes it possible to perform quite realistic simulations of radio pulses from air showers in a medium similar to the atmosphere but without variations of density with altitude. The effects of independently changing the density, the refractive index and the magnetic field strength are studied in the frequency domain for observers in the Cherenkov direction at far distances from the shower. This approach is particularly enlightening providing an explanation of the spectral behavior of the induced electric field in…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Radio Wave Propagation Studies
