The Payload for Ultrahigh Energy Observations (PUEO)
The Payload for Ultrahigh Energy Observations (PUEO) is a proposed balloon-borne NASA mission that will have world-leading sensitivity to the so-far undetected ultrahigh-energy (UHE) neutrino flux at energies above several EeV. PUEO would fly 40 km above the Antarctic continent and seeks to detect t...
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ftdatacite:10.5281/zenodo.4122991 2023-05-15T13:46:50+02:00 The Payload for Ultrahigh Energy Observations (PUEO) Deaconu, Cosmin 2020 https://dx.doi.org/10.5281/zenodo.4122991 https://zenodo.org/record/4122991 unknown Zenodo https://zenodo.org/communities/neutrino2020-posters https://dx.doi.org/10.5281/zenodo.4122992 https://zenodo.org/communities/neutrino2020-posters Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess CC-BY Text Poster article-journal ScholarlyArticle 2020 ftdatacite https://doi.org/10.5281/zenodo.4122991 https://doi.org/10.5281/zenodo.4122992 2021-11-05T12:55:41Z The Payload for Ultrahigh Energy Observations (PUEO) is a proposed balloon-borne NASA mission that will have world-leading sensitivity to the so-far undetected ultrahigh-energy (UHE) neutrino flux at energies above several EeV. PUEO would fly 40 km above the Antarctic continent and seeks to detect the impulsive Askaryan radio emission from the interactions of UHE neutrinos in Antarctic ice. PUEO builds on the experience of the successful ANtarctic Impulsive Transient Antenna (ANITA) program. With additional antennas, improved electronics, and a lower-threshold phased-array trigger, PUEO will have an order of magnitude more reach than ANITA at 10 EeV. PUEO is also sensitive to radio emission from extensive air showers, including upward-going showers initiated by taus from tau-neutrino interactions. Still Image Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic The Antarctic |
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DataCite Metadata Store (German National Library of Science and Technology) |
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The Payload for Ultrahigh Energy Observations (PUEO) is a proposed balloon-borne NASA mission that will have world-leading sensitivity to the so-far undetected ultrahigh-energy (UHE) neutrino flux at energies above several EeV. PUEO would fly 40 km above the Antarctic continent and seeks to detect the impulsive Askaryan radio emission from the interactions of UHE neutrinos in Antarctic ice. PUEO builds on the experience of the successful ANtarctic Impulsive Transient Antenna (ANITA) program. With additional antennas, improved electronics, and a lower-threshold phased-array trigger, PUEO will have an order of magnitude more reach than ANITA at 10 EeV. PUEO is also sensitive to radio emission from extensive air showers, including upward-going showers initiated by taus from tau-neutrino interactions. |
format |
Still Image |
author |
Deaconu, Cosmin |
spellingShingle |
Deaconu, Cosmin The Payload for Ultrahigh Energy Observations (PUEO) |
author_facet |
Deaconu, Cosmin |
author_sort |
Deaconu, Cosmin |
title |
The Payload for Ultrahigh Energy Observations (PUEO) |
title_short |
The Payload for Ultrahigh Energy Observations (PUEO) |
title_full |
The Payload for Ultrahigh Energy Observations (PUEO) |
title_fullStr |
The Payload for Ultrahigh Energy Observations (PUEO) |
title_full_unstemmed |
The Payload for Ultrahigh Energy Observations (PUEO) |
title_sort |
payload for ultrahigh energy observations (pueo) |
publisher |
Zenodo |
publishDate |
2020 |
url |
https://dx.doi.org/10.5281/zenodo.4122991 https://zenodo.org/record/4122991 |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_relation |
https://zenodo.org/communities/neutrino2020-posters https://dx.doi.org/10.5281/zenodo.4122992 https://zenodo.org/communities/neutrino2020-posters |
op_rights |
Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess |
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CC-BY |
op_doi |
https://doi.org/10.5281/zenodo.4122991 https://doi.org/10.5281/zenodo.4122992 |
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