Articles | Volume 38, issue 6
Ann. Geophys., 38, 1299–1312, 2020
https://doi.org/10.5194/angeo-38-1299-2020
Ann. Geophys., 38, 1299–1312, 2020
https://doi.org/10.5194/angeo-38-1299-2020

Regular paper 22 Dec 2020

Regular paper | 22 Dec 2020

Odd hydrogen response thresholds for indication of solar proton and electron impact in the mesosphere and stratosphere

Tuomas Häkkilä et al.

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ED: Publish subject to revisions (further review by editor and referees) (21 Sep 2020) by Petr Pisoft
AR by Tuomas Häkkilä on behalf of the Authors (21 Sep 2020)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (29 Sep 2020) by Petr Pisoft
RR by Anonymous Referee #2 (26 Oct 2020)
RR by Anonymous Referee #1 (02 Nov 2020)
ED: Publish as is (03 Nov 2020) by Petr Pisoft
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Short summary
The atmospheric impacts of energetic particle precipitation (EPP) can be useful in understanding the uncertainties of measuring the precipitation. Hence, information on how strong of an EPP flux has observable atmospheric impacts is needed. In this study, we find such threshold flux values using odd hydrogen concentrations from both satellite observations and model simulations. We consider the effects of solar proton events and radiation belt electron precipitation in the middle atmosphere.