Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause

We present a new model of the magnetospheric magnetic field. Using the finite element method, ChapmanFerraro problem is solved numerically in the considered approach. The whole magnetic field is a sum of: the dipole field, the field, produced by the internal current systems (cross-tail, Birkeland, r...

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Published in:Advances in Astronomy and Space Physics
Date:2011
Main Authors: Dobreva, P.S., Kartalev, M.D.
Format: Article
Language:English
Published: Advances in astronomy and space physics 2011
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/118974
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause / P.S. Dobreva, M.D. Kartalev // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 73-76. — Бібліогр.: 22 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-118974
record_format dspace
spelling Dobreva, P.S.
Kartalev, M.D.
2017-06-02T18:12:25Z
2017-06-02T18:12:25Z
2011
Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause / P.S. Dobreva, M.D. Kartalev // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 73-76. — Бібліогр.: 22 назв. — англ.
987-966-439-367-3
https://nasplib.isofts.kiev.ua/handle/123456789/118974
We present a new model of the magnetospheric magnetic field. Using the finite element method, ChapmanFerraro problem is solved numerically in the considered approach. The whole magnetic field is a sum of: the dipole field, the field, produced by the internal current systems (cross-tail, Birkeland, ring currents) and the field induced by the magnetopause currents. In contrast to similar earlier models, the internal magnetospheric magnetic fields are taken from Tsyganenko data-based model. The magnetosphere boundary could be arbitrary (generally non-axisymmetric). Input model parameters are the solar wind parameters, the Dst index and the dipole tilt angle. We discuss some results, obtained in three dimensional solution of the Neumann-Dirichlet problem corresponding to a closed magnetosphere.
We would like to thank the Bulgarian "Evrika" Foundation for financial support. This work is also supported by the European Social Fund and Bulgarian Ministry of Education, Youth and Science under Operative Program "Human Resources Development", Grant BG051PO001-3.3.04/40.
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Advances in astronomy and space physics
Advances in Astronomy and Space Physics
Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
spellingShingle Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
Dobreva, P.S.
Kartalev, M.D.
title_short Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
title_full Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
title_fullStr Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
title_full_unstemmed Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
title_sort numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause
author Dobreva, P.S.
Kartalev, M.D.
author_facet Dobreva, P.S.
Kartalev, M.D.
publishDate 2011
language English
container_title Advances in Astronomy and Space Physics
publisher Advances in astronomy and space physics
format Article
description We present a new model of the magnetospheric magnetic field. Using the finite element method, ChapmanFerraro problem is solved numerically in the considered approach. The whole magnetic field is a sum of: the dipole field, the field, produced by the internal current systems (cross-tail, Birkeland, ring currents) and the field induced by the magnetopause currents. In contrast to similar earlier models, the internal magnetospheric magnetic fields are taken from Tsyganenko data-based model. The magnetosphere boundary could be arbitrary (generally non-axisymmetric). Input model parameters are the solar wind parameters, the Dst index and the dipole tilt angle. We discuss some results, obtained in three dimensional solution of the Neumann-Dirichlet problem corresponding to a closed magnetosphere.
isbn 987-966-439-367-3
url https://nasplib.isofts.kiev.ua/handle/123456789/118974
citation_txt Numerical modeling of the magnetosphere with data based internal magnetic field and arbitrary magnetopause / P.S. Dobreva, M.D. Kartalev // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 73-76. — Бібліогр.: 22 назв. — англ.
work_keys_str_mv AT dobrevaps numericalmodelingofthemagnetospherewithdatabasedinternalmagneticfieldandarbitrarymagnetopause
AT kartalevmd numericalmodelingofthemagnetospherewithdatabasedinternalmagneticfieldandarbitrarymagnetopause
first_indexed 2025-12-07T18:59:59Z
last_indexed 2025-12-07T18:59:59Z
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