The Magnetospheric and Ionospheric Response to Solar Wind Dynamic Pressure Variations
- Gordon R. Wilson
Published Online: 18 MAR 2013
Copyright 1991 by the American Geophysical Union.
Modeling Magnetospheric Plasma Processes
How to Cite
Sibeck, D. G. (1991) The Magnetospheric and Ionospheric Response to Solar Wind Dynamic Pressure Variations, in Modeling Magnetospheric Plasma Processes (ed G. R. Wilson), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM062p0001
- Published Online: 18 MAR 2013
- Published Print: 1 JAN 1991
Print ISBN: 9780875900285
Online ISBN: 9781118663905
- Space plasmas—Mathematical models—Congresses;
- Magnetosphere—Mathematical models—Congresses
We discuss the characteristics of solar wind dynamic pressure variations associated with solar wind tangential discontinuties and transient processes at the Earth's bow shock. We quantify existing models for the transient magnetospheric and ionospheric response to the solar wind dynamic pressure variations. The largest variations in solar wind dynamic pressure drive large amplitude (∼1 RE magnetopause motion with radial velocities of ∼60 km s−1 and produce transient dayside ionospheric flows of 2 km s−1 which are organized into double convection vortices. Ground magnetometer signatures are most pronounced under the auroral ionosphere, where they reach 60–300 nT, and under the equatorial electrojet.