AIM-E: E-Region Auroral Ionosphere Model

The auroral oval is the high-latitude region of the ionosphere characterized by strong variability of its chemical composition due to precipitation of energetic particles from the magnetosphere. The complex nature of magnetospheric processes cause a wide range of dynamic variations in the auroral zo...

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Published in:Atmosphere
Main Authors: Vera Nikolaeva, Evgeny Gordeev, Tima Sergienko, Ludmila Makarova, Andrey Kotikov
Format: Article
Language:English
Published: MDPI AG 2021-06-01
Subjects:
Online Access:https://www.mdpi.com/2073-4433/12/6/748
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author Vera Nikolaeva
Evgeny Gordeev
Tima Sergienko
Ludmila Makarova
Andrey Kotikov
author_facet Vera Nikolaeva
Evgeny Gordeev
Tima Sergienko
Ludmila Makarova
Andrey Kotikov
author_sort Vera Nikolaeva
collection DOAJ
container_title Atmosphere
description The auroral oval is the high-latitude region of the ionosphere characterized by strong variability of its chemical composition due to precipitation of energetic particles from the magnetosphere. The complex nature of magnetospheric processes cause a wide range of dynamic variations in the auroral zone, which are difficult to forecast. Knowledge of electron concentrations in this highly turbulent region is of particular importance because it determines the propagation conditions for the radio waves. In this work we introduce the numerical model of the auroral E-region, which evaluates density variations of the 10 ionospheric species and 39 reactions initiated by both the solar extreme UV radiation and the magnetospheric electron precipitation. The chemical reaction rates differ in more than ten orders of magnitude, resulting in the high stiffness of the ordinary differential equations system considered, which was solved using the high-performance Gear method. The AIM-E model allowed us to calculate the concentration of the neutrals NO, N(<sup>4</sup>S), and N(<sup>2</sup>D), ions N<sup>+</sup>, N<sub>2</sub><sup>+</sup>, NO<sup>+</sup>, O<sub>2</sub><sup>+</sup>, O<sup>+</sup>(<sup>4</sup>S), O<sup>+</sup>(<sup>2</sup>D), and O<sup>+</sup>(<sup>2</sup>P), and electrons Ne, in the whole auroral zone in the 90‒150 km altitude range in real time. The model results show good agreement with observational data during both the quiet and disturbed geomagnetic conditions.
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spelling doaj-art-dec8020bcdf540d4a1e5e5d7ebccc8ae2025-08-20T00:17:14ZengMDPI AGAtmosphere2073-44332021-06-0112674810.3390/atmos12060748AIM-E: E-Region Auroral Ionosphere ModelVera Nikolaeva0Evgeny Gordeev1Tima Sergienko2Ludmila Makarova3Andrey Kotikov4Arctic and Antarctic Research Institute, 199397 Saint Petersburg, RussiaEarth’s Physics Department, Saint Petersburg State University, 199034 Saint Petersburg, RussiaSwedish Institute of Space Physics, 981 28 Kiruna, SwedenArctic and Antarctic Research Institute, 199397 Saint Petersburg, RussiaSaint Petersburg Branch of Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of Russian Academy of Sciences (IZMIRAN), 199034 Saint Petersburg, RussiaThe auroral oval is the high-latitude region of the ionosphere characterized by strong variability of its chemical composition due to precipitation of energetic particles from the magnetosphere. The complex nature of magnetospheric processes cause a wide range of dynamic variations in the auroral zone, which are difficult to forecast. Knowledge of electron concentrations in this highly turbulent region is of particular importance because it determines the propagation conditions for the radio waves. In this work we introduce the numerical model of the auroral E-region, which evaluates density variations of the 10 ionospheric species and 39 reactions initiated by both the solar extreme UV radiation and the magnetospheric electron precipitation. The chemical reaction rates differ in more than ten orders of magnitude, resulting in the high stiffness of the ordinary differential equations system considered, which was solved using the high-performance Gear method. The AIM-E model allowed us to calculate the concentration of the neutrals NO, N(<sup>4</sup>S), and N(<sup>2</sup>D), ions N<sup>+</sup>, N<sub>2</sub><sup>+</sup>, NO<sup>+</sup>, O<sub>2</sub><sup>+</sup>, O<sup>+</sup>(<sup>4</sup>S), O<sup>+</sup>(<sup>2</sup>D), and O<sup>+</sup>(<sup>2</sup>P), and electrons Ne, in the whole auroral zone in the 90‒150 km altitude range in real time. The model results show good agreement with observational data during both the quiet and disturbed geomagnetic conditions.https://www.mdpi.com/2073-4433/12/6/748auroral ovalE-region of ionospherenumerical modelingsubstormion compositionelectron concentration
spellingShingle Vera Nikolaeva
Evgeny Gordeev
Tima Sergienko
Ludmila Makarova
Andrey Kotikov
AIM-E: E-Region Auroral Ionosphere Model
auroral oval
E-region of ionosphere
numerical modeling
substorm
ion composition
electron concentration
title AIM-E: E-Region Auroral Ionosphere Model
title_full AIM-E: E-Region Auroral Ionosphere Model
title_fullStr AIM-E: E-Region Auroral Ionosphere Model
title_full_unstemmed AIM-E: E-Region Auroral Ionosphere Model
title_short AIM-E: E-Region Auroral Ionosphere Model
title_sort aim e e region auroral ionosphere model
topic auroral oval
E-region of ionosphere
numerical modeling
substorm
ion composition
electron concentration
url https://www.mdpi.com/2073-4433/12/6/748
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AT evgenygordeev aimeeregionauroralionospheremodel
AT timasergienko aimeeregionauroralionospheremodel
AT ludmilamakarova aimeeregionauroralionospheremodel
AT andreykotikov aimeeregionauroralionospheremodel