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- W2021825575 abstract "Abstract The concept of positive gradient in solar wind velocity with respect to the heliomagnetic latitude and the change in heliomagnetic latitude of Earth has been utilized to explain the differences in solar wind velocity variation around − and −/+ IMF sector boundaries in northern and southern heliolatitudes. It is shown that, using a sinusoidal symmetric heliospheric current sheet, one can explain the observed solar wind changes around the Hale and non-Hale types of sector boundaries." @default.
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- W2021825575 date "1986-09-01" @default.
- W2021825575 modified "2023-09-27" @default.
- W2021825575 title "On the cause of observed solar wind velocity variation around hale type sector boundary" @default.
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- W2021825575 doi "https://doi.org/10.1016/0032-0633(86)90084-x" @default.
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