On the possibility of using an electromagnetic ionosphere in global MHD simulations

Global magnetohydrodynamic (MHD) simulations of the Earth's magnetosphere must be coupled with a dynamical ionospheric module in order to give realistic results. The usual approach is to compute the field-aligned current (FAC) from the magnetospheric MHD variables at the ionospheric boundar...

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Main Author: P. Janhunen
Format: Article
Language:English
Published: Copernicus Publications 1998-04-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/16/397/1998/angeo-16-397-1998.pdf
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spelling doaj-fa5855f30bc74a618bdf9779dc7a4eea2020-11-24T21:12:43ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05761998-04-011639740210.1007/s00585-998-0397-yOn the possibility of using an electromagnetic ionosphere in global MHD simulationsP. Janhunen0Finnish Meteorological Institute, Geophysical Research, P.O. Box 503, FIN-00101 Helsinki, FinlandGlobal magnetohydrodynamic (MHD) simulations of the Earth's magnetosphere must be coupled with a dynamical ionospheric module in order to give realistic results. The usual approach is to compute the field-aligned current (FAC) from the magnetospheric MHD variables at the ionospheric boundary. The ionospheric potential is solved from an elliptic equation using the FAC as a source term. The plasma velocity at the boundary is the <b>E</b> × <b>B</b> velocity associated with the ionospheric potential. Contemporary global MHD simulations which include a serious ionospheric model use this method, which we call the electrostatic approach in this paper. We study the possibility of reversing the flow of information through the ionosphere: the magnetosphere gives the electric field to the ionosphere. The field is not necessarily electrostatic, thus we will call this scheme electromagnetic. The electric field determines the horizontal ionospheric current. The divergence of the horizontal current gives the FAC, which is used as a boundary condition for MHD equations. We derive the necessary formulas and discuss the validity of the approximations necessarily involved. It is concluded that the electromagnetic ionosphere-magnetosphere coupling scheme is a serious candidate for future global MHD simulators, although a few problem areas still remain. At minimum, it should be investigated further to discover whether there are any differences in the simulation using the electrostatic or the electromagnetic ionospheric coupling.<br><br><b>Key words.</b> Ionosphere · Ionosphere-magnetosphere interaction · Magnetospheric physics · Magnetosphere-ionosphere interaction · Space plasma physics · Numerical simulation studieshttps://www.ann-geophys.net/16/397/1998/angeo-16-397-1998.pdf
collection DOAJ
language English
format Article
sources DOAJ
author P. Janhunen
spellingShingle P. Janhunen
On the possibility of using an electromagnetic ionosphere in global MHD simulations
Annales Geophysicae
author_facet P. Janhunen
author_sort P. Janhunen
title On the possibility of using an electromagnetic ionosphere in global MHD simulations
title_short On the possibility of using an electromagnetic ionosphere in global MHD simulations
title_full On the possibility of using an electromagnetic ionosphere in global MHD simulations
title_fullStr On the possibility of using an electromagnetic ionosphere in global MHD simulations
title_full_unstemmed On the possibility of using an electromagnetic ionosphere in global MHD simulations
title_sort on the possibility of using an electromagnetic ionosphere in global mhd simulations
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 1998-04-01
description Global magnetohydrodynamic (MHD) simulations of the Earth's magnetosphere must be coupled with a dynamical ionospheric module in order to give realistic results. The usual approach is to compute the field-aligned current (FAC) from the magnetospheric MHD variables at the ionospheric boundary. The ionospheric potential is solved from an elliptic equation using the FAC as a source term. The plasma velocity at the boundary is the <b>E</b> × <b>B</b> velocity associated with the ionospheric potential. Contemporary global MHD simulations which include a serious ionospheric model use this method, which we call the electrostatic approach in this paper. We study the possibility of reversing the flow of information through the ionosphere: the magnetosphere gives the electric field to the ionosphere. The field is not necessarily electrostatic, thus we will call this scheme electromagnetic. The electric field determines the horizontal ionospheric current. The divergence of the horizontal current gives the FAC, which is used as a boundary condition for MHD equations. We derive the necessary formulas and discuss the validity of the approximations necessarily involved. It is concluded that the electromagnetic ionosphere-magnetosphere coupling scheme is a serious candidate for future global MHD simulators, although a few problem areas still remain. At minimum, it should be investigated further to discover whether there are any differences in the simulation using the electrostatic or the electromagnetic ionospheric coupling.<br><br><b>Key words.</b> Ionosphere · Ionosphere-magnetosphere interaction · Magnetospheric physics · Magnetosphere-ionosphere interaction · Space plasma physics · Numerical simulation studies
url https://www.ann-geophys.net/16/397/1998/angeo-16-397-1998.pdf
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