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Characteristics of low latitude boundary layer (LLBL) of the Earth's magnetosphere are investigated using data of Interball/Tail probe observations.
The most intensive energy transformation occurs over cusps and along the boundary between the mantle and low latitude boundary layer down to X= − 6 RE.
The results of experimental observations select two regions in the magnetospheric turbulent wake: plasma sheet and low latitude boundary layer (LLBL).
Low latitude boundary layer (LLBL) of the magnetosphere of the Earth is formed due to the mixing of magnetosheath and plasma sheet plasma.
We analyze plasma structures within the low latitude boundary layer (LLBL) observed by Interball Tail spacecraft under southward interplanetary magnetic field.
The thickness of the low latitude boundary layer (LLBL) is studied as a function of interplanetary magnetic field (IMF) using the data of THEMIS mission.
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Low-latitude boundary is at (pm 60^circ ).
This paper presents a statistical study of the high-latitude boundary layer (HLBL) performed on 53 Interball-1 magnetopause crossings.
These offsets are removed by zeroing drift values at the low-latitude boundary of the high-latitude convection pattern.
Both the along-track and cross-track components of the ion drift are expected to be zero at the low-latitude boundary of the convection zone.
Fig. 8 Dawn dusk (cross-tail) inflows in the current sheet of magnetotail are directed to the midnight from low-latitude boundary layer (LLBLs) of dawnside and duskside.
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