Statistics of plasma sheet convection

[ 43 ] For every RFE there was a thin auroral form aligned with the clockwise convection reversal, consistent with a converging electric field and an upward Birkeland current

Because plasma sheet convection is dominated by slow speed flows, a flow event was defined as a continuous block of samples during which β > 0.5 and the flow speed remained

[ 31 ] The majority of all earthward plasma sheet flow observations during all substorm phases consisted of slow speed (V < 100 km/s) flows, although the percentage was

Here we extend an earlier study of the proton aurora in the cusp during northward interplanetary magnetic field (IMF) conditions [Frey et al., 2002] to southward IMF conditions..

Pooled human EDTA plasma for assay calibration and linearity experiments was dialyzed three times (i.e., until the concentrations of choline, betaine, and DMG were below

Distinctive features of the CB event were the same as those during the Steady Magnetospheric Convection intervals: (1) wide double oval at the nightside; (2) thick plasma sheet,

However, the power output under ideal conditions in the wind tunnel was 28% lower than promised in the data sheet at rated wind speed.. The output was approximately 120 W

Under a northward IMF condition, magnetic reconnection is limited to a small high latitude region and K–H instability becomes important in bringing solar wind energy and plasma into