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- W2015370708 abstract "Several thousand magnetic measurements at distances from 3 to 10 RE from the database of Fairfield et al. [1994] have been used for studying the magnetic field response to variations of the hourly-averaged values of the solar wind dynamic pressure. The response differs from that predicted by the Mead [1964] model. Increase in the dynamic pressure compresses the magnetospheric field in the dayside sector mainly. In the most part of the nightside a depression dominates. The depression is connected with the growth of the cross-tail current." @default.
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- W2015370708 title "Three-dimensional magnetospheric response to variations in the solar wind dynamic pressure" @default.
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- W2015370708 doi "https://doi.org/10.1029/98gl00002" @default.
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