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Specific HESSI instrument performance parameters
are given in Table 2.
Table 2 HESSI Instrument Performance Parameters
| Number
of Germanium Detectors |
9
|
| Number
of Independent Detector Segments |
18
|
| Front
Segment Detector Diameter |
6.1 cm
|
| Rear
Segment Detector Diameter |
7.1 cm
|
| Front
Detector Segment Thickness |
1.5 cm
|
| Rear
Detector Segment Thickness |
6.5 cm
|
| Energy
Range |
3 keV to 15 MeV
|
| Energy
Resolution (FWHM) |
0.5 keV to 30 keV
increasing to 2 keV at 1 MeV,
5 keV at 15 MeV
|
| Imaging
Technique |
Fourier-transform imaging with
rotating modulation collimators
|
| Angular
Resolution |
2.3 arcsec to 40 (or 300) keV
7 arcsec to 400 keV
36 arcsec to 2.2 MeV
|
| FOV |
Full Sun
|
| Range
of Collimator Resolutions (FWHM) |
2.3 - 189 arcsec
|
| Time-averaged
Sensitive Area |
up to 118 cm2
|
| Temporal
Resolution |
Tens of ms for basic image
³ 2
s for detailed image
|
| Max Photon-tagged
Event Rate |
50,000 events/sec/segment
|
| Time
Resolution |
Events recorded with 1m
s relative,
1 ms absolute accuracy
|
| Attenuators |
On-board logic selects one of
4 states
|
| Rate
Mode |
Activated by on-board logic
|
3.1 Data Acquisition
The primary science data will be returned in event data packets,
indicated in Table 3 along with other packet types. The contents of these
packets include the time, energy and detector-segment identification of each
detected event. The relative time resolution of 1 m
s is sufficient that coincident events are indicated by identical time-tags,
instead of conventional flags. Aspect data from SAS and RAS are included
with sufficient time resolution that the instantaneous aspect associated
with each detected event can be inferred.
To help accommodate the large dynamic range expected
in flare count rates as a function of time and energy, instrument logic
will control the mechanical insertion of either or both of two x-ray attenuators
between the lower grids and detectors. As an additional measure, in large
flares, should the memory and/or data storage rates approach their limits,
on-board instrument logic will apply increasingly stringent energy criteria
to favor the retention of high energy photons, along with an unbiassed
subset of the more numerous low energy photons. At exceptionally high rates,
time-tagging of each detected event in the front segment detectors will
be replaced by recording in Fast Rate Counters with sufficient time resolution
to permit imaging, albeit with lower spectral resolution. In all cases,
Monitor Rates with lower time resolution are used to provide an overview
of detector performance and as input to support on-board decision-making.
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