Article ID Journal Published Year Pages File Type
1763310 Advances in Space Research 2016 11 Pages PDF
Abstract
The main generation mechanisms for the Earth's Low Latitude Boundary Layer (LLBL) are considered to be magnetic reconnection, viscous interactions such as Kelvin-Helmholtz instability and associated plasma mixing and diffusion. We have performed a statistical study of the Ultra Low Frequency (ULF) fluctuation power at the Pc4-Pc5 range using ≈6 years of THEMIS measurements of the plasma velocity and magnetic field. The results reveal a clear dawn-dusk asymmetry showing that the fluctuation power is typically more enhanced in the vicinity of the magnetopause downstream of the quasi-parallel shock. The statistical study of the Vx-component of the plasma velocity indicates that the LLBL is also thicker on the dawn-sector. These results may suggest that the physical mechanisms that provide power in the Pc4-Pc5 range are more effective on the dawn-sector and provide a means for a more effective LLBL generation.
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
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