Field-Aligned Radio Wave Propagation in the Plasmasphere Observed with IMAGE/RPI

Sales, G,  Huang, X,  Reinisch, B W,  Song, P,  Galkin, I,  Carpenter, D L, 
Fung, S F,  Benson, R F,  Green, J L,  Webb, P A

The IMAGE satellite is in an eccentric orbit that allows the satellite to move
from the magnetospheric cavity into the plasmasphere on each orbit. RPI radio
sounding made from the IMAGE satellite, as it approaches and recedes from the
plasmasphere, suggests that the predominantly observed echoes correspond to waves
propagating along the geomagnetic field lines. These echoes are frequently
observed on successive plasmagrams covering a period, on the average, of 8 to 10
minutes while the spacecraft moves a few thousand kilometers across the
geomagnetic field lines. Multiple echoes are often observed with time delays
corresponding to guided paths in both directions along the magnetic field in the
vicinity of L = 2 to 4. They appear to be a relatively consistent feature of the
plasmasphere/plasmapause region. The RPI three orthogonal-axis antenna systems
make it possible to determine the arrival angles of reflected signals. These
arrival angle calculations are made at each frequency for each echo within a
plasmagram using the received signal amplitude and phase on the three orthogonal
antennas. The measured angle-of-arrival is compared with the geomagnetic field
direction at the satellite using a dipole model of the earth's magnetic field.
The result of this comparison indicates that the echoes arrive from a direction
that is close to the model magnetic field direction at the satellite and are thus
consistent with the field-aligned propagation interpretation. From the available
RPI data for approximately 500 orbits acquired over a nine-month period,
statistics on the frequency of occurrence, duration, the location of these events
and length of the field-aligned propagation paths are presented.