Abstract--AGU Meeting December 1998 

High Angular Resolution Measurements of Geomagnetically Trapped Protons 

The Source/Loss-Cone Energetic Particle Spectrometer (SEPS) aboard the
POLAR spacecraft records ion angular distributions between 150 and 430
keV. Each of six detector units consists of a focal plane of solid-state
pixels mounted behind a pinhole aperture. Each pixel on the focal plane
records the particle flux at a single pitch angle with angular resolution
of 1.3 degrees. The field of view is about ±10 degrees about the central
axis. SEPS is mounted on the despun platform of the satellite and when
inside the magnetosphere the field of view usually includes the local
magnetic field direction and the trapped particle loss cone. During a
magnetic storm the ions can be examined to study the processes which
influence the angular distributions at small pitch angles These
processes include pitch angle scattering by waves, transport in L by
radial diffusion, and the removal of protons by charge exchange with the
hydrogen geocorona. Data will be shown for a magnetic storm in which ring
current ions are accelerated and redistributed into a non-equilibrium
profile.

Return to SEPPS Publications...