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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 signal 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 involved 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.


Zugehörige Institution(en) am KIT Institut für Astroteilchenphysik (IAP)
Publikationstyp Vortrag
Publikationsdatum 28.07.2023
Sprache Englisch
Identifikator KITopen-ID: 1000160826
HGF-Programm 51.13.03 (POF IV, LK 01) Kosmische Strahlung Auger
Veranstaltung 38th International Cosmic Ray Conference (ICRC 2023), Nagoya, Japan, 26.07.2023 – 03.08.2023
Bemerkung zur Veröffentlichung Plenary Talk
KIT – Die Forschungsuniversität in der Helmholtz-Gemeinschaft
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