Detection of the Cherenkov light diffused by Sea Water with the ULTRA Experiment
G.Agnetta (IASF-Palermo/INAF, Italy), P. Assis (LIP-Lisbon, Portugal),, B. Biondo (IASF-Palermo/INAF, Italy), P. Brogueira (LIP-Lisbon, Portugal), A., Cappa (IFSI-Torino/INAF & INFN-Torino, Italy), O. Catalano (IASF-Palermo/INAF, & INFN-Catania, Italy), J. Chauvin (LPSC-Grenoble

TL;DR
This paper presents the ULTRA experiment's measurements of Cherenkov light diffusion by sea water, aiding ultra-high-energy cosmic ray detection and improving shower reconstruction for space-based observatories.
Contribution
It provides the first measurements of sea water's diffusing properties for Cherenkov light, addressing a key gap in cosmic ray observation techniques.
Findings
Measured sea water diffusion coefficient for Cherenkov light
Determined the energy threshold for detection in sea water
Demonstrated the feasibility of using sea water reflections for cosmic ray studies
Abstract
The study of Ultra High Energy Cosmic Rays represents one of the most challenging topic in the Cosmic Rays and in the Astroparticle Physics fields. The interaction of primary particles with atmospheric nuclei produces a huge Extensive Air Shower together with isotropic emission of UV fluorescence light and highly directional Cherenkov photons, that are reflected/diffused isotropically by the impact on the Earth's surface or on high optical depth clouds. For space-based observations, detecting the reflected Cherenkov signal in a delayed coincidence with the fluorescence light improves the accuracy of the shower reconstruction in space and in particular the measurement of the shower maximum, giving a strong signature for discriminating hadrons and neutrinos, and helping to estimate the primary chemical composition. Since the Earth's surface is mostly covered by water, the ULTRA (UV Light…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Radiation Detection and Scintillator Technologies
