7 citations · 7 across the 9 of their papers we have counts for
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Reconstruction of anomalous air showers with SKA-Low
Vital De Henau, Sjoerd Bouma, Justin Bray +31
Double-bump showers are a surprising class of extensive air showers (EAS) predicted by Monte Carlo simulations, which, so far, no experiment has been able to directly detect. They…
Anomalous Air Showers and What They Reveal About Hadronic Interactions and Cosmic-ray Masses
Stijn Buitink, Vital De Henau, Sjoerd Bouma +28
The identification of the sources and acceleration mechanisms of cosmic rays require precise measurements of their mass composition. Currently, the most reliable method is to measu…
Measuring High-Energy Cosmic Particles with the SKA
Tim Huege, Katharine Mulrey, Sjoerd Bouma +28
The origin of high-energy cosmic rays remain one of astrophysics' greatest unsolved mysteries. SKA-Low will be able to measure air showers initiated by cosmic rays with unprecedent…
Origins of Cosmic Rays in the Galactic-extragalactic Transition Energy Range
A. Corstanje, S. Saha, S. Bouma +28
Cosmic rays arrive at Earth with energies ranging from to over eV. One of the open questions in high-energy cosmic ray science concerns the origin of the highest-e…
Using SKA-Low to Detect PeV Gamma-rays from Galactic Sources
Anna Nelles, Philipp Laub, Haoning He +28
Detecting so called PeVatrons is considered one of the prime goals of -ray astronomy. PeVatrons are astrophysical objects in the Galaxy that are sources of cosmic rays exceeding…
Investigating double bump air showers with the SKA-Low
V. De Henau, S. Bouma, J. Bray +30
Double-bump showers are a rare class of extensive air showers (EAS) predicted by Monte Carlo simulations. They occur when a high-energy secondary particle, the leading particle, tr…
Minimal prospects for radio detection of extensive air showers in the atmosphere of Jupiter
J. D. Bray, A. Nelles
One possible approach for detecting ultra-high-energy cosmic rays and neutrinos is to search for radio emission from extensive air showers created when they interact in the atmosph…