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- W2002167364 abstract "The excitation mechanism of the upstream low‐frequency waves (0.01–0.05 Hz) is investigated based on the wave observations. We compared the observed wave frequencies with the frequencies expected from the ion (proton) beam‐cyclotron instability process. We estimated the beam velocity from the solar wind parameters using Sonnerup’s formula. Our analysis supports the hypothesis that these waves are excited by the resonant beam‐cyclotron instability. For the waves observed in the deep foreshock region, however, we found it necessary to include the solar wind convection effect on the wave propagation." @default.
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- W2002167364 title "On the excitation mechanism of the low-frequency upstream waves" @default.
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- W2002167364 doi "https://doi.org/10.1029/ja089ia08p06623" @default.
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