Open questions in cosmic-ray research at ultrahigh energies

R Alves Batista, J Biteau, M Bustamante… - Frontiers in Astronomy …, 2019 - frontiersin.org
We review open questions and prospects for progress in ultrahigh-energy cosmic ray
(UHECR) research, based on a series of discussions that took place during the “The High …

[HTML][HTML] Cosmic-ray extremely distributed observatory

P Homola, D Beznosko, G Bhatta, Ł Bibrzycki… - Symmetry, 2020 - mdpi.com
The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a newly formed, global
collaboration dedicated to observing and studying cosmic rays (CR) and cosmic-ray …

POEMMA: probe of extreme multi-messenger astrophysics

AV Olinto, JH Adams, R Aloisio… - arxiv preprint arxiv …, 2017 - arxiv.org
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) mission is being designed
to establish charged-particle astronomy with ultra-high energy cosmic rays (UHECRs) and to …

Cosmic ray detection in space

M Boezio, R Munini, P Picozza - Progress in Particle and Nuclear Physics, 2020 - Elsevier
Cosmic rays are energetic particles composed primarily of protons and helium nuclei but
including, with varying abundances, all atomic nuclei species, electrons and even …

Status of the K-EUSO orbital detector of ultra-high energy cosmic rays

P Klimov, M Battisti, A Belov, M Bertaina, M Bianciotto… - Universe, 2022 - mdpi.com
K-EUSO (KLYPVE-EUSO) is a planned orbital mission aimed at studying ultra-high energy
cosmic rays (UHECRs) by detecting fluorescence and Cherenkov light emitted by extensive …

A Review of the EUSO-Balloon Pathfinder for the JEM-EUSO Program

JH Adams Jr, S Ahmad, D Allard, A Anzalone… - Space Science …, 2022 - Springer
EUSO-Balloon is a pathfinder for JEM-EUSO, the mission concept of a spaceborne
observatory which is designed to observe Ultra-High Energy Cosmic Ray (UHECR)-induced …

Sensitivity of a proposed space-based Cherenkov astrophysical-neutrino telescope

A Neronov, DV Semikoz, LA Anchordoqui, JH Adams… - Physical Review D, 2017 - APS
Neutrinos with energies in the PeV to EeV range produce upgoing extensive air showers
when they interact underground close enough to the surface of the Earth. We study the …

[HTML][HTML] Remote sensing of the atmosphere by the ultraviolet detector TUS onboard the Lomonosov satellite

P Klimov, B Khrenov, M Kaznacheeva, G Garipov… - Remote Sensing, 2019 - mdpi.com
The orbital detector TUS (Tracking Ultraviolet Setup) with high sensitivity in near-visible
ultraviolet (tens of photons per time sample of 0.8 μ s of wavelengths 300–400 nm from a …

Cosmic ray oriented performance studies for the JEM-EUSO first level trigger

G Abdellaoui, S Abe, A Acheli, JH Adams Jr… - Nuclear Instruments and …, 2017 - Elsevier
JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and
Neutrinos (E> 5⋅ 1 0 19 eV) from the International Space Station (ISS). Looking down from …

First results from the TUS orbital detector in the extensive air shower mode

BA Khrenov, PA Klimov, MI Panasyuk… - … of Cosmology and …, 2017 - iopscience.iop.org
Abstract TUS (Tracking Ultraviolet Set-up), the first orbital detector of extreme energy cosmic
rays (EECRs), those with energies above 50 EeV, was launched into orbit on April 28, 2016 …