作者: C. Peymirat , D. Fontaine , C. Senior
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摘要: Pressure gradients created by the adiabatic convection of magnetospheric plasma cannot completely explain observed distribution at planetary scale region 2 field-aligned currents. The contribution particle loss processes is evaluated. assumption a strong pitch-angle diffusion for both ions and electrons shown to provide estimates comparable fluxes soft precipitations. efficiency ion charge exchange generally found be weak relative precipitation. These terms are included into simplified fluid model transport. agreement with observations reveals importance losses, especially in generation currents