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Solar Wind Control of Daytime, Midperiod Geomagnetic Pulsations

  • E. W. Greenstadt
  • R. L. McPherron
  • K. Takahashi
Part of the Advances in Earth and Planetary Sciences book series (AEPS, volume 11)

Abstract

Numerous studies have established that various properties of geomagnetic pulsations are linked to various properties of the solar wind. The linkage in most cases is rather loose, suggesting that combinations of factors must be involved in generation and control of pulsation activity. We review briefly the most significant observational results and we describe and discuss critically the two most prominent models for external generation of magnetospheric waves. We present arguments favoring joint application of the models, wherein perturbations in the magnetosheath resulting from favorable interplanetary field orientation are delivered to the magnetopause, transferred directly into the subsolar magnetosphere, and amplified into surface waves on the flank of the magnetosphere by Kelvin-Helmholtz instability at high solar wind speed. This combination of circumstances can account for experimental correlations of pulsation occurrence with interplanetary field orientation, periods with interplanetary field strength, and amplitudes with solar wind velocity.

Keywords

Solar Wind Interplanetary Magnetic Field Cone Angle Solar Wind Speed Solar Wind Velocity 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Center for Academic Publications Japan 1981

Authors and Affiliations

  • E. W. Greenstadt
    • 1
  • R. L. McPherron
    • 2
  • K. Takahashi
    • 2
  1. 1.Space Sciences DepartmentTRW Defense and Space Systems GroupRedondo BeachUSA
  2. 2.Institute of Geophysics and Planetary PhysicsUniversity of CaliforniaLos AngelesUSA

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