Normal data acquisition is based on storage of
the energy and arrival time of every detected photon, together with instrument
SAS and RAS aspect information. These data are stored in the spacecraft’s
4 Gbyte mass memory until telemetered. Ground data systems will convert
these data into X-ray and g-ray
images and spectra.
An 11-m ground station from Allied Signal and EMP,
currently under construction at UCB, will provide command transmission
and data reception. The Mission Operations Center and Science Operations
Center at UCB will operate the spacecraft and instrument, write the data
onto CD-ROMs, and distribute the data to the Solar Data Analysis Center
(SDAC) at GSFC and the High Energy Data Center (HEDC) in Zurich. The SDAC
will archive and distribute both data and analysis software to outside
users in the U.S., and coordinate access to context observations from other
spacecraft and ground instruments. The HEDC will perform the same functions
in Europe. A program of ground observations is supported directly by HESSI
to provide the most critical context data. All users will have equal access
to the ground-based data.
3.0 Science Instrumentation
The HESSI scientific objectives will be achieved
with high resolution imaging spectroscopy observations from soft X-rays
to g -rays, using
a single instrument consisting of an Imaging System, a Spectrometer, and
Instrument Electronics. The Imaging System is made up of nine Rotating
Modulation Collimators (RMCs), each consisting of a pair of widely separated
grids mounted on the rotating spacecraft. Pointing information is provided
by the Solar Aspect System (SAS) and Roll Angle System (RAS).
The Spectrometer has nine segmented GeDs, one behind
each RMC, to detect photons from 3 keV to 15 MeV. Each detector is made
from a single germanium crystal, which is electrically divided into independent
front and rear segments to provide an optimum response for low and high
energy photons, respectively. The GeDs are cooled to <~75 K by a space-qualified
long-life mechanical cryocooler to achieve the highest spectral resolution
(Table 2) of any presently available g
-ray detector. As the spacecraft rotates, the RMCs convert the spatial
information from the source into temporal modulation of the photon counting
rates of the GeDs. The Instrument Electronics amplify, shape, and digitize
the GeD signals, provide low-voltage power and GeD high voltage, format
the data, and interface to the spacecraft electronics.