Impact of Ionospheric Ions on Magnetospheric Dynamics

Elena A. Kronberg, Elena E. Grigorenko, Raluca Ilie, Lynn Kistler, Dan Welling

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

Ionospheric ion outflow changes the magnetospheric dynamics. It is especially important during disturbed magnetospheric conditions. In the inner magnetosphere, it is relevant also during quiet times. The presence of ionospheric ions affects the plasma properties by changing the plasma density, temperature, and pressure. Modified plasma properties then influence the magnitude of Alfvén velocity, affect the structure and dynamics of the current sheet, and, as a result, physical processes such as reconnection, the development of plasma instabilities, and wave generation. On the large scales, the ionospheric ion outflow changes the shape of the magnetosphere and its configuration. Outflow affects substorm-like events, magnetic storms, dynamics of radiation belts, and magnetosphere- ionosphere-ring current coupling. In this chapter, we introduce the circulation of ionospheric ions and then discuss the effects mentioned above in detail. We pose questions for future research.

Original languageEnglish (US)
Title of host publicationMagnetospheres in the Solar System
PublisherWiley
Pages353-364
Number of pages12
ISBN (Electronic)9781119815624
ISBN (Print)9781119507529
DOIs
StatePublished - Jan 1 2021
Externally publishedYes

Keywords

  • ionospheric ions
  • magnetic storms
  • magnetospheric dynamics
  • plasma density
  • plasma properties
  • space weather
  • substorm-like events

ASJC Scopus subject areas

  • General Energy

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