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- W1953262107 abstract "Abstract Sheared plasma flows at the low‐latitude boundary layer (LLBL) correlate well with early afternoon auroral arcs and upward field‐aligned currents. We present a simple analytic model that relates solar wind and ionospheric parameters to the strength and thickness of field‐aligned currents (Λ) in a region of sheared velocity, such as the LLBL. We compare the predictions of the model with DMSP observations and find remarkably good scaling of the upward region 1 currents with solar wind and ionospheric parameters in region located at the boundary layer or open field lines at 1100–1700 magnetic local time. We demonstrate that and Λ ∼ L when Λ/ L < 5 where L is the auroral electrostatic scale length. The sheared boundary layer thickness (Δ m ) is inferred to be around 3000 km, which appears to have weak dependence on V sw . J ∥ has dependencies on Δ m , Σ p , n sw , and V sw . The analytic model provides a simple way to organize data and to infer boundary layer structures from ionospheric data." @default.
- W1953262107 created "2016-06-24" @default.
- W1953262107 creator A5041761983 @default.
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- W1953262107 date "2015-05-01" @default.
- W1953262107 modified "2023-10-14" @default.
- W1953262107 title "The dependence of the strength and thickness of field‐aligned currents on solar wind and ionospheric parameters" @default.
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- W1953262107 doi "https://doi.org/10.1002/2014ja020312" @default.
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