GSTDTAP  > 气候变化
DOI10.1029/2018GL079421
Ionization of the Polar Atmosphere by Energetic Electron Precipitation Retrieved From Balloon Measurements
Mironova, I. A.1; Artamonov, A. A.2; Bazilevskaya, G. A.3; Rozanov, E. V.4,5,6; Kovaltsov, G. A.7; Makhmutov, V. S.3; Mishev, A. L.8,9; Karagodin, A. V.1
2019-01-28
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2019
卷号46期号:2页码:990-996
文章类型Article
语种英语
国家Russia; Switzerland; Finland
英文摘要

We retrieve ionization rates in the atmosphere caused by energetic electron precipitation from balloon observations in the polar atmosphere and compare them against ionization rates recommended for the Phase 6 of the Coupled Model Intercomparison Project. In our retrieval procedure, we consider the precipitating electrons with energies from about tens of keV to 5 MeV. Our simulations with 1-D radiative-convective model with interactive neutral and ion chemistry show that the difference of the Phase 6 of the Coupled Model Intercomparison Project and balloon-based ionization rate can lead to underestimation of the NOx enhancement by more than 100% and ozone loss up to 25% in the mesosphere. The atmospheric response is different below 50 km due to considering highly energetic electrons, but it is not important because the absolute values of atmospheric impact is tiny. Ionization rates obtained from the balloon observations reveal a high variability.


Plain Language Summary The main idea of our manuscript is to demonstrate that the atmospheric ionization rates (IR) can be successfully retrieved from the long-term balloon observations of the energetic electron precipitation (EEP) events and used to evaluate the uncertainties of the other IR data sets, for example, IR recommended for the Phase 6 of the Coupled Model Intercomparison Project (CMIP6). IR obtained from the balloon observations reveal a high variability. This means that the time resolution used in CMIP6 probably is not enough to consider high frequency variability of the precipitating electron fluxes. Using 1-D radiative-convective model with neutral and ion chemistry, we compared the atmospheric response to the one particular EEP observed by balloons and presented in CMIP6 data. We show that the difference of the CMIP6 and balloon-based IRs can lead to underestimation of the NOx enhancement by more than 100% and ozone loss by up to 25% in the mesosphere. Our results are new and needed for the understanding of the potential uncertainties in CMIP6 EEP forcing. Our paper will give inspiration for the continuation of the balloon measurements of EEP-related processes using improved instruments.


领域气候变化
收录类别SCI-E
WOS记录号WOS:000458607400051
WOS关键词MIDDLE ATMOSPHERE ; MODEL ; RADIATION ; CRACEPII ; PARTICLE
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
被引频次:24[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/28142
专题气候变化
作者单位1.St Petersburg State Univ, Dept Phys Earth, Fac Phys, St Petersburg, Russia;
2.Fed Biomed Agcy Russia, Res Inst Space Med, Fed Res Clin Ctr, Moscow, Russia;
3.Russian Acad Sci, Lebedev Phys Inst, Moscow, Russia;
4.WRC, PMOD, Davos, Switzerland;
5.ETHZ, IAC, Davos, Switzerland;
6.Russian Acad Sci, Pushkov Inst Terr Magnetism Ionosphere & Radio Wa, Western Dept, Kaliningrad, Russia;
7.Ioffe Phys Tech Inst, St Petersburg, Russia;
8.Univ Oulu, Space Climate Res Unit, Oulu, Finland;
9.Sodankyla Geophys Observ, Oulu, Finland
推荐引用方式
GB/T 7714
Mironova, I. A.,Artamonov, A. A.,Bazilevskaya, G. A.,et al. Ionization of the Polar Atmosphere by Energetic Electron Precipitation Retrieved From Balloon Measurements[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(2):990-996.
APA Mironova, I. A..,Artamonov, A. A..,Bazilevskaya, G. A..,Rozanov, E. V..,Kovaltsov, G. A..,...&Karagodin, A. V..(2019).Ionization of the Polar Atmosphere by Energetic Electron Precipitation Retrieved From Balloon Measurements.GEOPHYSICAL RESEARCH LETTERS,46(2),990-996.
MLA Mironova, I. A.,et al."Ionization of the Polar Atmosphere by Energetic Electron Precipitation Retrieved From Balloon Measurements".GEOPHYSICAL RESEARCH LETTERS 46.2(2019):990-996.
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