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- W1553658794 abstract "The low latitude boundary layer (LLBL) is a region where solar wind momentum and energy is transferred to the magnetosphere. Enhanced broadband electric plasma waves from <5 Hz to 10 5 Hz and magnetic waves from <5 Hz to the electron cyclotron frequency are characteristic of the LLBL. Analyses of Polar plasma waves show that these broadband waves are actually discrete electrostatic and electromagnetic modes as well as solitary bipolar pulses (electron holes). It is noted that all wave modes can be generated by ∼100 eV to ∼10 keV auroral electrons and protons. We will review wave-particle interactions, with focus on cross-diffusion rates and the contributions of such interactions toward the formation of the boundary layer. In summary, we will present a scenario where the global solar wind-magnetosphere interaction is responsible for the auroral zone particle beams, and hence for the generation of plasma waves and the formation of the boundary layer. It is speculated that all planetary magnetospheres will have boundary layers and they will be characterized by similar currents and plasma wave modes." @default.
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- W1553658794 date "2003-01-01" @default.
- W1553658794 modified "2023-10-03" @default.
- W1553658794 title "ELF/VLF plasma waves in the low latitude boundary layer" @default.
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- W1553658794 doi "https://doi.org/10.1029/133gm19" @default.
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