Radio detection of cosmic-ray air showers with the OVRO-LWA: status and future plans.
A. Romero-Wolf*, R. Monroe, G. Hallinan, W. Carvalho, K. Plant, K. Belov, A. Nelles, M. Eastwood, M. Anderson, L. D'Addario, J. Kocz and D. Woody
Pre-published on:
July 22, 2019
Published on:
July 02, 2021
Abstract
We present the successful radio frequency (30 - 80 MHz) self-triggered detection and identification of 10 high energy cosmic rays with Caltech's Owens Valley Radio Observatory Long Wavelength Array (OVRO-LWA). The core of the OVRO-LWA consists of 256 dual-polarization antennas that are approximately evenly spaced in a 200 m diameter disk with several outliers at longer distances. Based on this success we present future plans for an array covering a 2.5 km diameter area for measuring the flux and composition of cosmic rays in the $3\times10^{16}$ eV - $10^{18}$ eV energy band.
DOI: https://doi.org/10.22323/1.358.0405
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating
very compact bibliographies which can be beneficial to authors and
readers, and in "proceeding" format
which is more detailed and complete.