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- W2074266200 abstract "Multi-spacecraft observations in the interplanetary space are used to build up a picture of the distribution of solar wind velocities in heliographic latitude and longitude. Analyses are made for the solar wind data obtained by Sakigake, Suisei, IMP-8 and Giotto between late 1985 and early 1987. Until Janaury 1986, high-speed streams were extended across the equator from the high latitudes of the heliosphere. After March 1986, high-speed streams were rarely seen on the equator. Although there remained a slight wavy pattern in latitude-longitude structure, low-speed streams were basically ranged along the equator. After January 1987, the amplitude of this wavy pattern was further diminished and low-speed regions were completely aligned to the equator." @default.
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- W2074266200 date "1988-12-01" @default.
- W2074266200 modified "2023-09-26" @default.
- W2074266200 title "Multi-spacecraft observations of heliographic structure of the solar wind speed" @default.
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- W2074266200 doi "https://doi.org/10.1016/0032-0633(88)90003-7" @default.
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