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- W2076758030 abstract "Determining the shape of the magnetopause is one of the oldest problems in space physics and one of its earliest success stories. Chapman and Ferraro [1931] were the first to recognize that the Earth's magnetic field carves out a cavity in the oncoming solar wind. Theoretical studies based on gas dynamics which predicted the shape of the magnetopause bounding this cavity [e.g., Ferraro, 1960; Spreiter and Hyett, 1963] were followed by studies demonstrating that magnetopause crossings generally occur in the expected locations [Ness, 1965]. Some years passed before it was realized that the orientation of the interplanetary magnetic field (IMF) also has an important effect on the size and shape of the magnetosphere [Aubry et al, 1970]. Determining the location and shape of the magnetopause is useful for both practical and theoretical reasons. The magnetic field rotates from magnetosheath to magnetospheric orientations at the magnetopause. Since some satellites in geosynchronous orbit make attitude adjustments by applying magnetic torques using the ambient field, it is important to know whether the magnetopause is Earthward or Sunward of the satellite. An accurate knowledge of the magnetopause location may help in planning data acquisition during forthcoming missions which lack the resources to take continuous observations. Analytical modellers of the magnetospheric magnetic field wish to confine-that field within a well-determined magnetopause boundary. Finally, changes in the magnetopause location and shape reveal important information about solar wind and magnetospheric conditions." @default.
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- W2076758030 date "1995-01-01" @default.
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- W2076758030 title "Demarcating the magnetopause boundary" @default.
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- W2076758030 doi "https://doi.org/10.1029/95rg00285" @default.
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