PDMP Page 8

 

                                   

      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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This page last updated: June 27, 2008