Exceptional middle latitude electron precipitation detected by balloon observations : implications for atmospheric composition |
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Author: | Mironova, Irina1; Sinnhuber, Miriam2; Bazilevskaya, Galina3; |
Organizations: |
1Earth Physics Department, Faculty of Physics, St. Petersburg State University, St. Petersburg, Russia 2Institute of Meteorology and Climate Research, Karlsruhe Institute of Technology, Karlsruhe, Germany 3Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia
4British Antarctic Survey, Cambridge, United Kingdom
5Instituto de Astrofisica de Andalucia, CSIC, Granada, Spain 6Moscow Institute of Physics and Technology, Moscow, Russia 7PMOD/WRC and IAC ETHZ, Davos, Switzerland 8Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA USA 9Institute of Meteorology and Climatology, University of Natural Resources and Life Sciences, Vienna, Austria 10Sodankylä Geophysical Observatory, Sodankylä, Finland |
Format: | article |
Version: | published version |
Access: | open |
Online Access: | PDF Full Text (PDF, 2.7 MB) |
Persistent link: | http://urn.fi/urn:nbn:fi-fe2022113068142 |
Language: | English |
Published: |
Copernicus Publications,
2022
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Publish Date: | 2022-11-30 |
Description: |
AbstractEnergetic particle precipitation leads to ionization in the Earth’s atmosphere, initiating the formation of active chemical species which destroy ozone and have the potential to impact atmospheric composition and dynamics down to the troposphere. We report on one exceptionally strong high-energy electron precipitation event detected by balloon measurements in geomagnetic midlatitudes on 14 December 2009, with ionization rates locally comparable to strong solar proton events. This electron precipitation was possibly caused by wave–particle interactions in the slot region between the inner and outer radiation belts, connected with still poorly understood natural phenomena in the magnetosphere. Satellite observations of odd nitrogen and nitric acid are consistent with widespread electron precipitation into magnetic midlatitudes. Simulations with a 3D chemistry–climate model indicate the almost complete destruction of ozone in the upper mesosphere over the region where high-energy electron precipitation occurred. Such an extraordinary type of energetic particle precipitation can have major implications for the atmosphere, and their frequency and strength should be carefully studied. see all
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Series: |
Atmospheric chemistry and physics |
ISSN: | 1680-7316 |
ISSN-E: | 1680-7324 |
ISSN-L: | 1680-7316 |
Volume: | 22 |
Issue: | 10 |
Pages: | 6703 - 6716 |
DOI: | 10.5194/acp-22-6703-2022 |
OADOI: | https://oadoi.org/10.5194/acp-22-6703-2022 |
Type of Publication: |
A1 Journal article – refereed |
Field of Science: |
115 Astronomy and space science |
Subjects: | |
Funding: |
This research has been supported by the Russian Foundation for Basic Research (grant no. 20-55-12020), the Deutsche Forschungsgemeinschaft (grant no. SI 1088/7-1), the Russian Science Foundation (grant no. 20-67-46016) and the Ministry of Science and Higher Education of the Russian Federation (grant no. 075-15-2021-583). |
Copyright information: |
© Author(s) 2022. This work is distributed under the Creative Commons Attribution 4.0 License. |
https://creativecommons.org/licenses/by/4.0/ |