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Effect of change in large and fast solar wind dynamic pressure on geosynchronous magnetic field
Authors:N L Borodkov  Liu Jing-Bo  Huang Zhao-Hui  G N Zastenker  Wang Chi and P E Eiges
Affiliation:Space Research Institute, Moscow, Russia; State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences,Beijing 100080, China
Abstract:We present a comparison of changes in large and sharp solar wind dynamic pressure, observed by several spacecraft, with fast disturbances in the magnetospheric magnetic field, measured by the geosynchronous satellites. More than 260 changes in solar wind pressure during the period 1996--2003 are selected for this study. Large statistics show that an increase (a decrease) in dynamic pressure always results in an increase (a decrease) in the magnitude of geosynchronous magnetic field. The amplitude of response to the geomagnetic field strongly depends on the location of observer relative to the noon meridian, the value of pressure before disturbance, and the change in amplitude of pressure.
Keywords:solar wind dynamic pressure changes  geosynchronous magnetic field
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