We have constructed and tested a prototype instrument for space plasma phys
ics research. The instrument is capable of measuring total ion velocity dis
tribution functions as well as velocity distribution functions for individu
al mass-per-charge (m/q) species. The instrument consists of a deflection s
ystem, a toroidal energy-per-charge (E/q) analyzer, and a hemispherical con
denser that serves either as the second stage of E/q analysis or as a gated
time-of-flight velocity filter. The deflection system subtends a full 360
degrees in azimuth and allows one to select ions for analysis in the toroid
al section according to their elevation angle with respect to the axis of t
he instrument. The hemispherical condenser accepts a fraction of the ions t
ransmitted by the toroidal analyzer through an electronic shutter at its en
trance plane. With the shutter open, total ion distribution functions are m
easured. By appropriately gating the shutter and measuring the time of flig
ht of ions introduced into the hemisphere, ion velocities are measured and
m/q determined. The dimensions of the instrument have been chosen for measu
rements of the interplanetary solar wind at distances of 4-20 solar radii (
R-sun) from the surface of the sun, consistent with the requirements of a s
olar probe mission. It can also be adapted to make measurements at 1 a.u. (
C) 1999 American Institute of Physics. [S0034-6748(99)04907-2].