Macroscopic approach to the radar echo scatter from high-energy particle cascades

To probe the cosmic particle flux at the highest energies, large volumes of dense material like ice have to be monitored. This can be achieved by exploiting the radio signal. In this work, we provide a macroscopic model to predict the radar echo signatures found when a radio signal is reflected from...

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Veröffentlicht in:	arXiv.org 2024-06
Hauptverfasser:	E Huesca Santiago, de Vries, K D, Allison, P, Beatty, J, Besson, D, Connolly, A, Cummings, A, Deaconu, C, De Kockere, S, Frikken, D, Hast, C, C -Y Kuo, Kyriacou, A, Latif, U A, Loudon, I, Lukic, V, McLennan, C, Mulrey, K, Nam, J, Nivedita, K, Nozdrina, A, Oberla, E, Prohira, S, Ralston, J P, Seikh, M F H, Stanley, R S, Stoffels, J, Toscano, S, Van den Broeck, D, N van Eijndhoven, Wissel, S
Format:	Artikel
Sprache:	eng
Schlagworte:	Cosmic rays Echo scatter Macroscopic models Neutrinos Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Radar echoes Radar signatures Radio signals Scattering Signal strength
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