The present study attempts to analyze the average ring current density
and pressure in the magnetospheric equatorial plane (as a function of
geocentric distance and local time) based on the AMPTE/CCE-CHEM proto
n distributions according to two different AE ranges, corresponding to
a low (AE<100 nT) and a moderate (100 nT<AE<600 nT) geomagnetic or au
roral activity. In order to obtain a statistically significant databas
e for a high spatial resolution, the data were averaged over 2 years.
The results provide a trend of the ring current and show its general a
verage features as a function of geomagnetic activity. In particular,
the total ring current is dominated by the pressure gradient term, res
ulting in an eastward current in the inner magnetosphere (L<4.5) and a
n extended westward current at higher altitudes. The westward current
is always stronger than the eastward current. Moreover, the ring curre
nt system is a function of magnetic local time, exhibiting a noon-midn
ight asymmetry in general, as well as a function of geomagnetic activi
ty exhibiting an enhancement of about 20% during active times (in midn
ight-dusk region only). The location of the total current peak in the
midnight sector is at about MLT=23 00, and its changes with magnetic a
ctivity are interpreted as an effect of the particles injection from t
he tail during the storms/substorms. The derived current values are co
mpared to previous model predictions and observations.