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.

Original languageEnglish
Pages (from-to)990-996
Number of pages7
JournalGeophysical Research Letters
Volume46
Issue number2
Early online date16 Jan 2019
DOIs
StatePublished - 28 Jan 2019

    Scopus subject areas

  • Geophysics
  • Earth and Planetary Sciences(all)

    Research areas

  • atmospheric response, balloon measurements, EEP CMIP6, energetic electron precipitation (EEP), ionization rates, polar atmosphere, PARTICLE, CRACEPII, MIDDLE ATMOSPHERE, MODEL, RADIATION

ID: 37491346