Ionization effect in the Earth’s atmosphere due to cosmic rays during the GLE<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si11.svg"><mml:mrow><mml:mo>#</mml:mo></mml:mrow></mml:math>71 on 17 May 2012

Pätsi, Susanna; Mishev, Alexander

doi:10.1016/j.asr.2022.02.008

Cited by 5 publications

(1 citation statement)

References 63 publications

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“…In order to realistically quantify the terrestrial effects of the precipitating high-energy SEPs, specifically for atmospheric physics and chemistry studies, we normalized the ion production rate to a given period, namely to 24 hours, employing the recombination model by Krivolutsky et al (2006) and assuming isotropic distribution (Pätsi and Mishev 2022), that is, we computed the 24h averaged ionization effect similarly to Velinov 2018, 2020). Employment of an isotropic distribution during these computations is reasonable, because of the wide angular distribution of incoming SEPs and none the least the fast isotropization of the event.…”

Section: Atmospheric Ionization Effectmentioning

confidence: 99%

NMDB@Athens

2023

Cosmic Ray Studies With Neutron Detectors

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This volume documents the papers presented at the hybrid symposium on cosmic ray studies with neutron monitors in Athens in September 2022. The contributions are dedicated to six topics: cosmic rays in the heliosphere, GLE analysis and space weather research, cosmic rays and the Earth's atmosphere, instrumentation and stability of neutron detectors, their response functions, and the data bases and catalogues of the Real-Time database for high resolution Neutron Monitor measurements (NMDB) project, which are freely accessible to a large user community.

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Section: Atmospheric Ionization Effectmentioning

confidence: 99%