JOURNAL OF GEOPHYSICAL RESEARCH, VOL 104, No. A1, PAGES 429-436, JANUARY 1, 1999
Simulation of off-equatorial ring current ion spectra measured by POLAR for
a moderate storm at solar minimum
V.K. Jordanova1, C.J. Farrugia1, J.M. Quinn1,
R.B. Torbert1, J.E. Borovsky2, R.B. Sheldon3, and
W.K. Peterson4
Abstract. We use our kinetic drift-loss model to sutdy ring current dynamics
during moderate geomagnetic activity at the minimum phase of the current solar cycle,
on March 20-22, 1996. Interplanetary conditions monitored by Wind during
this period show fluctuations about zero in the (GSM) Bz component,
which are due to Alfven waves in a stream-stream interaction region. The corresponding
Dst index shows general activity punctuated by 2 moderate storms (min Dst~-50 nT
and ~-70 nT, respectively) of ~15 hours duration each. We calculate the off-equatorial ring
current proton spectra in the energy range 100 ev to 300 keV and compare them with
measurements provided by the HYDRA, TIMAS, and CEPPAD instruments on the Polar spacecraft
at MLT~2 and MLT~14. We find reasonable overall agreement. An eastward offset of 3 hours in the
Kp-dependent Volland-Stern convection electric field with gamma=2 is necessary in order to
match modeled with observed dips in the energy spectra. Collisional losses have larger
effect on the postnoon spectra and reduce significantly the low-energy proton distribution
at low L shells and at higher magnetic latitudes. These losses reach
maximum values for slowly drifting (~2--10 keV) particles. Our study suggests
that a more realistic magnetospheric electric field and additional diffusion processes
should be considered to reduce the overestimated width and depth of the dip in the
modeled dayside spectra.