A Surface Radio Array for the Enhancement of IceTop and its Science Prospects
Radio detection of air showers in the current era has progressed immensely to effectively extract the properties of these air showers. Primary cosmic rays with energies of hundreds of PeV have been successfully measured with the method of radio detection. There are also attempts to observe high-ener...
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ftdatacite:10.48550/arxiv.1907.04171 2023-05-15T18:22:32+02:00 A Surface Radio Array for the Enhancement of IceTop and its Science Prospects V., Aswathi Balagopal Haungs, Andreas Huber, Thomas Huege, Tim Kleifges, Matthias Renschler, Max Schieler, Harald Schröder, Frank G. Weindl, Andreas 2019 https://dx.doi.org/10.48550/arxiv.1907.04171 https://arxiv.org/abs/1907.04171 unknown arXiv https://dx.doi.org/10.1051/epjconf/201921604004 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2019 ftdatacite https://doi.org/10.48550/arxiv.1907.04171 https://doi.org/10.1051/epjconf/201921604004 2022-03-10T16:43:00Z Radio detection of air showers in the current era has progressed immensely to effectively extract the properties of these air showers. Primary cosmic rays with energies of hundreds of PeV have been successfully measured with the method of radio detection. There are also attempts to observe high-energy neutrinos with this technique. Current radio experiments measuring cosmic-ray air showers mostly operate in the frequency range of 30-80 MHz. An optimization of the frequency band of operation can be done for maximizing the signal-to-noise ratio that can be achieved by an array of radio antennas at the South Pole, operated along with IceTop. Such an array can improve the reconstruction of air showers performed with IceTop. The prospect of using such an optimized radio array for measuring gamma rays of PeV energies from the Galactic Center is discussed. : To be published in the proceedings of the ARENA2018 conference Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
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Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences V., Aswathi Balagopal Haungs, Andreas Huber, Thomas Huege, Tim Kleifges, Matthias Renschler, Max Schieler, Harald Schröder, Frank G. Weindl, Andreas A Surface Radio Array for the Enhancement of IceTop and its Science Prospects |
topic_facet |
Instrumentation and Methods for Astrophysics astro-ph.IM High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
Radio detection of air showers in the current era has progressed immensely to effectively extract the properties of these air showers. Primary cosmic rays with energies of hundreds of PeV have been successfully measured with the method of radio detection. There are also attempts to observe high-energy neutrinos with this technique. Current radio experiments measuring cosmic-ray air showers mostly operate in the frequency range of 30-80 MHz. An optimization of the frequency band of operation can be done for maximizing the signal-to-noise ratio that can be achieved by an array of radio antennas at the South Pole, operated along with IceTop. Such an array can improve the reconstruction of air showers performed with IceTop. The prospect of using such an optimized radio array for measuring gamma rays of PeV energies from the Galactic Center is discussed. : To be published in the proceedings of the ARENA2018 conference |
format |
Article in Journal/Newspaper |
author |
V., Aswathi Balagopal Haungs, Andreas Huber, Thomas Huege, Tim Kleifges, Matthias Renschler, Max Schieler, Harald Schröder, Frank G. Weindl, Andreas |
author_facet |
V., Aswathi Balagopal Haungs, Andreas Huber, Thomas Huege, Tim Kleifges, Matthias Renschler, Max Schieler, Harald Schröder, Frank G. Weindl, Andreas |
author_sort |
V., Aswathi Balagopal |
title |
A Surface Radio Array for the Enhancement of IceTop and its Science Prospects |
title_short |
A Surface Radio Array for the Enhancement of IceTop and its Science Prospects |
title_full |
A Surface Radio Array for the Enhancement of IceTop and its Science Prospects |
title_fullStr |
A Surface Radio Array for the Enhancement of IceTop and its Science Prospects |
title_full_unstemmed |
A Surface Radio Array for the Enhancement of IceTop and its Science Prospects |
title_sort |
surface radio array for the enhancement of icetop and its science prospects |
publisher |
arXiv |
publishDate |
2019 |
url |
https://dx.doi.org/10.48550/arxiv.1907.04171 https://arxiv.org/abs/1907.04171 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1051/epjconf/201921604004 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1907.04171 https://doi.org/10.1051/epjconf/201921604004 |
_version_ |
1766201942597435392 |