This study suggests that Kelvin-Helmholtz waves can be a somewhat common, and possibly constant, instrument for the entrance of solar wind into terrestrial magnetospheres under various IMF orientations.
2.
The research characterized variances in formation of the interplanetary magnetic field ( IMF ) largely influenced by Kelvin-Helmholtz waves ( which occur at the interface of two fluids ) as a result of differences in thickness and numerous other characteristics of the boundary layer.
3.
Experts believe that this was the first occasion that the appearance of Kelvin-Helmholtz waves at the magnetopause had been displayed at high latitude dawnward orientation of the IMF . These waves are being seen in unforeseen places under solar wind conditions that were formerly believed to be undesired for their generation.
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