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Atmospheric Monitoring for Astroparticle Physics Observatories

Keilhauer, Bianca ORCID iD icon 1
1 Institut für Astroteilchenphysik (IAP), Karlsruher Institut für Technologie (KIT)

Abstract (englisch):

For many observatories recording high-energy cosmic rays, gamma rays, or neutrinos, the Earth’s atmosphere is either an integral part or at least a considerable aspect of the detector setup. After giving an overview of the influence of the atmosphere and its variability on the development of the observed particle cascades and the signals detected from them, atmospheric monitoring strategies implemented by the different observatories are described. Examples of the impact of atmospheric parameters and profiles on the core data of these observatories are given and technical aspects of long-term and partially very laborious monitoring efforts of the Earth’s atmosphere are discussed. Due to the per se interdisciplinary character of atmospheric monitoring in astroparticle physics, several new projects beyond the core physics of the astroparticle physics observatories have evolved and some are reviewed in this presentation.


Verlagsausgabe §
DOI: 10.5445/IR/1000163997
Veröffentlicht am 10.11.2023
Cover der Publikation
Zugehörige Institution(en) am KIT Institut für Astroteilchenphysik (IAP)
Publikationstyp Proceedingsbeitrag
Publikationsjahr 2023
Sprache Englisch
Identifikator ISSN: 1824-8039
KITopen-ID: 1000163997
HGF-Programm 51.13.03 (POF IV, LK 01) Kosmische Strahlung Auger
Erschienen in 38th International Cosmic Ray Conference (ICRC2023) - Review Talks
Veranstaltung 38th International Cosmic Ray Conference (ICRC 2023), Nagoya, Japan, 26.07.2023 – 03.08.2023
Verlag Scuola Internazionale Superiore di Studi Avanzati (SISSA)
Seiten Art.-Nr.: 021
Serie Proceedings of Science ; 444
Vorab online veröffentlicht am 27.10.2023
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