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KIMIE (KInetic Model of Ionospheric Electrons) is a 1D kinetic model developed by Garcia and Forme (2009).
There is a great demand for a proper model of ionospheric irregularity specification based on GNSS TEC measurements.
Therefore, if a model of ionospheric and magnetospheric currents (such as CM4) cannot be used, leveling methods are required to reduce the effect of temporal variation.
Six years of the hand-scaled ionospheric characteristics from December 2002 to December 2008 were used to build a local empirical model of ionospheric electron density (LEMI) for Irkutsk.
We then obtain the global distribution of ionospheric potential, utilizing a thin shell model, based on integration along field lines of the current continuity equation with a realistic model of ionospheric conductivity.
The empirical model of ionospheric irregularities based on ROTI data is actually for space weather studies and transionospheric radio propagation applications, i.e., estimation, specification, and prediction of the probability and area of ionospheric irregularity development and their dependence on solar and geomagnetic activity.
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assimilative modeling of ionospheric electrodynamics.
This study presents the modeling of ionospheric response to geomagnetic storms of September 9 14, 2005.
The coefficient of whistler reflection and its variation were calculated both analytically for simplified models and numerically for more realistic models of ionospheric altitude electron distributions.
Methods such as that of Kamide, Richmond, and Matsushita (called KRM) (Ahn et al. 1995) and assimilative modeling of ionospheric electrodynamics (AMIE) (Richmond 1992) allow determination of electrodynamic quantities of the upper atmosphere, and models exist for the entire near-Earth system with input from the solar wind (Ridley et al. 2002).
This paper presents the model simulation results of ionospheric E-region parameters during geomagnetic storm on May 2 3, 2010.
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