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Ionization of the Polar Atmosphere by Energetic Electron Precipitation Retrieved From Balloon Measurements
Author(s) -
Mironova I. A.,
Artamonov A. A.,
Bazilevskaya G. A.,
Rozanov E. V.,
Kovaltsov G. A.,
Makhmutov V. S.,
Mishev A. L.,
Karagodin A. V.
Publication year - 2019
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2018gl079421
Subject(s) - ionization , atmosphere (unit) , electron precipitation , electron , atmospheric sciences , ion , physics , electron ionization , environmental science , radiative transfer , atomic physics , polar , atmospheric physics , computational physics , meteorology , plasma , astronomy , nuclear physics , magnetosphere , quantum mechanics
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 N O x 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.