Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere
In this paper we develop a new method for the analysis of excitation and propagation of planetary electromagnetic waves (PEMW) in the ionosphere of the Earth. The nonlinear system of equations for PEMW, valid for any height, from D to F regions, including intermediate altitudes between D and E an...
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Format: | Article |
Language: | English |
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Copernicus Publications
2014-04-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/32/449/2014/angeo-32-449-2014.pdf |
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author | Yu. Rapoport Yu. Selivanov V. Ivchenko V. Grimalsky E. Tkachenko A. Rozhnoi V. Fedun |
author_facet | Yu. Rapoport Yu. Selivanov V. Ivchenko V. Grimalsky E. Tkachenko A. Rozhnoi V. Fedun |
author_sort | Yu. Rapoport |
collection | DOAJ |
description | In this paper we develop a new method for the analysis of excitation and
propagation of planetary electromagnetic waves (PEMW) in the ionosphere of
the Earth. The nonlinear system of equations for PEMW, valid for any height,
from D to F regions, including intermediate altitudes between D and E and
between E and F regions, is derived. In particular, we have found the system
of nonlinear one-fluid MHD equations in the β-plane approximation valid
for the ionospheric F region (Aburjania et al., 2003a, 2005). The
series expansion in a "small" (relative to the local geomagnetic field)
non-stationary magnetic field has been applied only at the last step of the
derivation of the equations. The small mechanical vertical displacement of
the media is taken into account. We have shown that obtained equations can be
reduced to the well-known system with Larichev–Reznik vortex solution in the
equatorial region (see e.g. Aburjania et al., 2002). The excitation of
planetary electromagnetic waves by different initial perturbations has been
investigated numerically. Some means for the PEMW detection and data
processing are discussed. |
first_indexed | 2024-12-19T00:49:25Z |
format | Article |
id | doaj.art-43f27451dc4a4d58a47094d03868922a |
institution | Directory Open Access Journal |
issn | 0992-7689 1432-0576 |
language | English |
last_indexed | 2024-12-19T00:49:25Z |
publishDate | 2014-04-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Annales Geophysicae |
spelling | doaj.art-43f27451dc4a4d58a47094d03868922a2022-12-21T20:44:07ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762014-04-013244946310.5194/angeo-32-449-2014Excitation of planetary electromagnetic waves in the inhomogeneous ionosphereYu. Rapoport0Yu. Selivanov1V. Ivchenko2V. Grimalsky3E. Tkachenko4A. Rozhnoi5V. Fedun6Kyiv National Taras Shevchenko University, 2, Glushkova Av., Build. 1, 03680 Kyiv, UkraineSpace Research Institute NASU-NSAU, 40, Glushkov Av., 03680, Kiev 187, UkraineKyiv National Taras Shevchenko University, 2, Glushkova Av., Build. 1, 03680 Kyiv, UkraineUniversity of Morelos, Av. Universidad, 1001, Z.P. 62210, Cuernavaca, Morelos, MexicoKyiv National Taras Shevchenko University, 2, Glushkova Av., Build. 1, 03680 Kyiv, UkraineInstitute of Physics of the Earth, Russian Academy of Sciences, 10 B. Gruzinskaya, Moscow, 123995, RussiaSpace Systems Laboratory, Department of Automatic Control and Systems Engineering, University of Sheffield, Sheffield, S1 3JD, UKIn this paper we develop a new method for the analysis of excitation and propagation of planetary electromagnetic waves (PEMW) in the ionosphere of the Earth. The nonlinear system of equations for PEMW, valid for any height, from D to F regions, including intermediate altitudes between D and E and between E and F regions, is derived. In particular, we have found the system of nonlinear one-fluid MHD equations in the β-plane approximation valid for the ionospheric F region (Aburjania et al., 2003a, 2005). The series expansion in a "small" (relative to the local geomagnetic field) non-stationary magnetic field has been applied only at the last step of the derivation of the equations. The small mechanical vertical displacement of the media is taken into account. We have shown that obtained equations can be reduced to the well-known system with Larichev–Reznik vortex solution in the equatorial region (see e.g. Aburjania et al., 2002). The excitation of planetary electromagnetic waves by different initial perturbations has been investigated numerically. Some means for the PEMW detection and data processing are discussed.https://www.ann-geophys.net/32/449/2014/angeo-32-449-2014.pdf |
spellingShingle | Yu. Rapoport Yu. Selivanov V. Ivchenko V. Grimalsky E. Tkachenko A. Rozhnoi V. Fedun Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere Annales Geophysicae |
title | Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere |
title_full | Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere |
title_fullStr | Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere |
title_full_unstemmed | Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere |
title_short | Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere |
title_sort | excitation of planetary electromagnetic waves in the inhomogeneous ionosphere |
url | https://www.ann-geophys.net/32/449/2014/angeo-32-449-2014.pdf |
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