EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation

The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) experiment will make new measurements from suborbital space as a precursor for future space missions that will address the challenge of the extremely low fluxes of ultra-high energy cosmic rays (UHECR) and very high ene...

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Main Authors: Cummings Austin, Eser Johannes, Filippatos George, Olinto Angela, Venters Tonia, Wiencke Lawrence
Format: Article
Language:English
Published: EDP Sciences 2023-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2023/09/epjconf_uhecr2023_06009.pdf
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author Cummings Austin
Eser Johannes
Filippatos George
Olinto Angela
Venters Tonia
Wiencke Lawrence
author_facet Cummings Austin
Eser Johannes
Filippatos George
Olinto Angela
Venters Tonia
Wiencke Lawrence
author_sort Cummings Austin
collection DOAJ
description The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) experiment will make new measurements from suborbital space as a precursor for future space missions that will address the challenge of the extremely low fluxes of ultra-high energy cosmic rays (UHECR) and very high energy (VHE) neutrinos. The EUSO-SPB2 detector is comprised of two 1m diameter aperture telescopes. The Fluorescence Telescope (FT) will point in nadir and will record fluorescence light from cosmic ray EAS with energies above 1 EeV in its field of view of 36 by 12 degrees. The Cherenkov Telescope (CT) features a silicon photomultiplier focal surface with a field of view of 12 by 6 degrees. The CT will switch between two observation modes: one which points the CT above the limb to measure the Cherenkov emission of cosmic ray EAS with energies above 1 PeV and one which points the CT below the limb to record the Cherenkov emission produced by PeV scale EAS initiated by neutrino-sourced tau decay. As it is the first time such an instrument has been flown, one of the priorities of the CT will be the study of the optical background for observing neutrinos in this way. EUSO-SPB2 is undergoing the final integration steps for launch on a NASA super pressure balloon payload in the spring of 2023 from Wanaka NZ. The CT was field-tested in March 2022 and the FT in August - September 2022. The data collected during the EUSO-SPB2 mission will be essential to advancing the development of a space-based multi-messenger observatory such as the Probe of Extreme Multi-Messenger Astrophysics (POEMMA). In this contribution, we discuss the EUSO-SPB2 science goals, the instruments, the expected performance and the current status.
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spelling doaj.art-56b9294b3c9640218c01b39586d0c6b82023-06-09T09:15:59ZengEDP SciencesEPJ Web of Conferences2100-014X2023-01-012830600910.1051/epjconf/202328306009epjconf_uhecr2023_06009EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observationCummings Austin0Eser Johannes1Filippatos George2Olinto Angela3Venters Tonia4Wiencke Lawrence5Departments of Physics and Astronomy & Astrophysics, Institute for Gravitation and the Cosmos, Pennsylvania State UniversityDepartment of Astrophysics & Astronomy, The University of ChicagoDepartment of Physcis, Colorado School of MinesDepartment of Astrophysics & Astronomy, The University of ChicagoNASA Goddard Space Flight CenterDepartment of Physcis, Colorado School of MinesThe Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) experiment will make new measurements from suborbital space as a precursor for future space missions that will address the challenge of the extremely low fluxes of ultra-high energy cosmic rays (UHECR) and very high energy (VHE) neutrinos. The EUSO-SPB2 detector is comprised of two 1m diameter aperture telescopes. The Fluorescence Telescope (FT) will point in nadir and will record fluorescence light from cosmic ray EAS with energies above 1 EeV in its field of view of 36 by 12 degrees. The Cherenkov Telescope (CT) features a silicon photomultiplier focal surface with a field of view of 12 by 6 degrees. The CT will switch between two observation modes: one which points the CT above the limb to measure the Cherenkov emission of cosmic ray EAS with energies above 1 PeV and one which points the CT below the limb to record the Cherenkov emission produced by PeV scale EAS initiated by neutrino-sourced tau decay. As it is the first time such an instrument has been flown, one of the priorities of the CT will be the study of the optical background for observing neutrinos in this way. EUSO-SPB2 is undergoing the final integration steps for launch on a NASA super pressure balloon payload in the spring of 2023 from Wanaka NZ. The CT was field-tested in March 2022 and the FT in August - September 2022. The data collected during the EUSO-SPB2 mission will be essential to advancing the development of a space-based multi-messenger observatory such as the Probe of Extreme Multi-Messenger Astrophysics (POEMMA). In this contribution, we discuss the EUSO-SPB2 science goals, the instruments, the expected performance and the current status.https://www.epj-conferences.org/articles/epjconf/pdf/2023/09/epjconf_uhecr2023_06009.pdf
spellingShingle Cummings Austin
Eser Johannes
Filippatos George
Olinto Angela
Venters Tonia
Wiencke Lawrence
EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation
EPJ Web of Conferences
title EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation
title_full EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation
title_fullStr EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation
title_full_unstemmed EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation
title_short EUSO-SPB2: A balloon experiment for UHECR and VHE neutrino observation
title_sort euso spb2 a balloon experiment for uhecr and vhe neutrino observation
url https://www.epj-conferences.org/articles/epjconf/pdf/2023/09/epjconf_uhecr2023_06009.pdf
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