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In addition, majority of substorms occurred during low or moderate solar wind streams.
Intense relativistic electron flux variations have also been noted during high-speed solar wind streams (HSSs) (Paulikas and Blake 1979).
The variability manifested as solar flares, CMEs, SEPs, and high-speed solar wind streams directly affects space weather on short time scales.
Brecht (1997) showed that the precipitation of slow solar wind streams, i.e. low energy protons, is favored in the hemisphere; this is in agreement with our results.
The occurrence of scintillation peaked on days with high-speed solar wind streams (HSS) or with CME impacts at the Earth's magnetosphere.
Typically, global Pc5 waves are observed during high solar wind streams, and they are about an order of magnitude more intense than common Pc5 pulsations.
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All the so-called people, wind streaming from their faces.
A solar flare or high-speed solar wind stream creates a high-pressure region in the solar wind.
The sudden increase in the speed of a large wind stream, especially in the tropics, can also cause surges.
high-speed solar wind stream.
Such storms often follow from the interaction of a fast solar wind stream or an interplanetary magnetic cloud.
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