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Modeling of the Ionospheric Current System and Calculating Its Contribution to the Earth’s Magnetic Field

  • Boris E. Prokhorov
  • Matthias Förster
  • Vincent Lesur
  • Alexander A. Namgaladze
  • Matthias Holschneider
  • Claudia Stolle
Part of the Astrophysics and Space Science Library book series (ASSL, volume 448)

Abstract

The additional magnetic field produced by the ionospheric current system is a part of the Earth’s magnetic field. This current system is a highly variable part of a global electric circuit. The solar wind and interplanetary magnetic field (IMF) interaction with the Earth’s magnetosphere is the external driver for the global electric circuit in the ionosphere. The energy is transferred via the field-aligned currents (FACs) to the Earth’s ionosphere. The interactions between the neutral and charged particles in the ionosphere lead to the so-called thermospheric neutral wind dynamo which represents the second important driver for the global current system. Both processes are components of the magnetosphere–ionosphere–thermosphere (MIT) system, which depends on solar and geomagnetic conditions, and have significant seasonal and UT variations.

The modeling of the global dynamic Earth’s ionospheric current system is the first aim of this investigation. For our study, we use the Potsdam version of the Upper Atmosphere Model (UAM-P). The UAM is a first-principle, time-dependent, and fully self-consistent numerical global model. The model includes the thermosphere, ionosphere, plasmasphere, and inner magnetosphere as well as the electrodynamics of the coupled MIT system for the altitudinal range from 80 (60) km up to the 15 Earth radii. The UAM-P differs from the UAM by a new electric field block. For this study, the lower latitudinal and equatorial electrodynamics of the UAM-P model was improved.

The calculation of the ionospheric current system’s contribution to the Earth’s magnetic field is the second aim of this study. We present the method, which allows computing the additional magnetic field inside and outside the current layer as generated by the space current density distribution using the Biot-Savart law. Additionally, we perform a comparison of the additional magnetic field calculation using 2D (equivalent currents) and 3D current distribution.

Notes

Acknowledgements

This work was partially supported by Deutsche Forschungsgemeinschaft (DFG).

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Copyright information

© Springer International Publishing AG 2018

Authors and Affiliations

  • Boris E. Prokhorov
    • 1
  • Matthias Förster
    • 1
  • Vincent Lesur
    • 2
  • Alexander A. Namgaladze
    • 3
  • Matthias Holschneider
    • 4
  • Claudia Stolle
    • 1
  1. 1.GFZ German Research Centre for GeosciencesHelmholtz Centre PotsdamPotsdamGermany
  2. 2.Institut de Physique du Globe de ParisSorbonne Paris Cité, Université Paris-DiderotParisFrance
  3. 3.Murmansk Arctic State UniversityMurmanskRussia
  4. 4.Institute of Applied MathematicsUniversity of PotsdamPotsdamGermany

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