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- W2105372523 abstract "Low-altitude spacecraft on magnetotail field lines often detect a distinctive signature in the precipitating ion flux. A velocity-dispersed ion structure is often observed near the poleward boundary of the auroral oval. At the low-latitude edge of this structure an absence of precipitating ions is seen, previously referred to as “the gap,” separating the velocity-dispersed ions at the higher latitudes from the more diffuse, plasma sheet-like ions at lower latitudes. We present a model of low-altitude particle precipitation that reproduces these observed features in the ion spectra and provides a quantitative estimate of the downtail plasma sheet properties. The model calculations are compared with observations from the Akebono spacecraft. In this model, the dispersed ion velocity signature maps to a region in the distant plasma sheet where the plasma has a field-aligned bulk flow. The gap maps to a region in the distant magnetotail where the ion fluxes are below the detection threshold of the instrument, due to the low plasma sheet density and temperature in that region." @default.
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- W2105372523 date "1995-04-01" @default.
- W2105372523 modified "2023-10-14" @default.
- W2105372523 title "Low altitude signature of the plasma sheet boundary layer: Observations and model" @default.
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- W2105372523 doi "https://doi.org/10.1029/95gl00304" @default.
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