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- W2183624203 abstract "Studies of the solar wind-magnetosphere interaction often rely on L1 observations that are propagated toward the Earth. The propagation techniques are based on an assumption of a negligible evolution of upstream parameters along the solar wind path. This study uses multi-point observations in the solar wind with the motivation to check this assumption. The data measured in the L1 point by ACE are propagated and compared with observations of the THEMIS spacecraft orbiting in the near-Earth space. A special attention is paid to the region in front of the Earth's bow shock (foreshock) because reflected and accelerated particles not only excite the waves of large amplitudes but they can modify mean values of quantities measured in an un-perturbed solar wind." @default.
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- W2183624203 date "2010-01-01" @default.
- W2183624203 modified "2023-10-09" @default.
- W2183624203 title "Evolution of the Solar Wind Speed from the L1 to Earth" @default.
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