E. Mobius et al., The Solar Energetic Particle Ionic Charge Analyzer (SEPICA) and the data processing unit (S3DPU) for SWICS, SWIMS and SEPICA, SPACE SCI R, 86(1-4), 1998, pp. 449-495
The Solar Energetic Particle Ionic Charge Analyzer (SEPICA) ir; the main in
strument on the Advanced Composition Explorer (ACE) to determine the ionic
charge states of solar and interplanetary energetic particles in the energy
range from approximate to 0.2 MeV nucl(-1) to approximate to 5 MeV charge(
-1). The charge state of energetic ions contains key information to unravel
source temperatures, acceleration, fractionation and transport processes f
or these particle populations. SEPICA will have the ability to resolve indi
vidual charge states and have a substantially larger geometric factor than
its predecessor ULEZEQ on ISEE-1 and -3, on which SEPICA is based. To achie
ve these two requirements at the same time, SEPICA is composed of one high-
charge resolution sensor section and two Low-charge resolution, but large g
eometric factor sections. The charge resolution is achieved by the focusing
of the incoming ions, through a multi-slit mechanical collimator, deflecti
on in an electrostatic analyzer with a voltage up to 30 kV, and measurement
of the impact position in the detector system. To determine the nuclear ch
arge (element) and energy of the incoming ions, the combination of thin-win
dow Bow-through proportional counters with isobutane as counter gas and ion
-implanted solid state detectors provide for 3 independent Delta E (energy
loss) versus E (residual energy) telescopes. The multi-wire proportional co
unter simultaneously determines the energy loss Delta E and the impact posi
tion of the ions. Suppression of background fi om penetrating cosmic radiat
ion is provided by an anti-coincidence system with a CsI scintillator and S
i-photodiodes, The data are compressed and formatted in a data processing u
nit (S3DPU) that also handles the commanding and various automatted functio
ns of the instrument. The S3BPU ir shared with the Solar Wind Ten Charge Sp
ectrometer (SWICS) and the Solar Wind ion Mass Spectrometer (SWIMS) and thu
s provides the same services for three of the ACE instruments. It has evolv
ed out of a lone family of data. processing units for particle spectrometer
s.