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- W4238889223 abstract "Extended periods of very low geomagnetic activity as described by very quiet intervals (VQI’s) occur only at those times when the solar wind velocity V has a generally decreasing trend, i.e., they mainly occur either after the velocity peak of a high speed solar stream has passed the Earth, or at times when the Earth is immersed in a low speed solar plasma provided that the daily mean value of dV/dt is negative. The VQI’s most frequently start when dV/dt < 0 and dB z /dt > 0 (B z is the geocentric solar magnetrospheric-GSM Z-component of the IMF) and end most likely when dV/dt > 0 and dB z /dt < 0. The temporal trends of the solar wind (SW) velocity affect the variation of the a p index only when the level of geomagnetic activity is generally low. It is suggested that a gradual expansion or contraction of the magnetosphere, associated with a slow variation of the SW pressure, plays a role in the modification of the reconnection-driven magnetohydrodynamic (MHD) fluctuations in the magnetosphere." @default.
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- W4238889223 date "1989-01-01" @default.
- W4238889223 modified "2023-10-03" @default.
- W4238889223 title "Very Quiet Intervals of Geomagnetic Activity and the Solar Wind Structure" @default.
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- W4238889223 doi "https://doi.org/10.1007/978-3-0348-9280-3_3" @default.
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