XTE
X-ray Timing Explorer, Also called RXTE (
Bruno B. Rossi X-ray Timing
Explorer)
Cost: $195 million, Launched under the MELVS contract
Delta's new avionics system will use an array of redundant laser gyros and
accelerometers to sense the vehicle's velocity and attitude movement, which
includes its angular position and direction. The avionics system feeds data to
onboard computers which control Delta 2's engines and power, engine start, main
engine cutoff, staging and payload separation. The avionics system now has two
power sources and is completely redundant. If one data system is lost, the
other will complete the mission.
http://heasarc.gsfc.nasa.gov/docs/xte/
sat-index articles
Built under coordination of NASA-Goddard Space Flight Center. It
includes two high gain antennae, allowing an almost continuous telemetry stream
using
TDRS's
Multiple Access mode.
Instrument with large collecting area but low spatial resolution, for
accurate timing and spectral measurements of bright X-ray sources. Built by the
LHEA at GSFC
The PCA is an array of five proportional counters with a total collecting area
of 6500 square cm. The instrumental properties are:
Energy
range
|
2
- 60 keV
|
Energy
resolution
|
&<
18% at 6 keV
|
Time
resolution
|
1
microsec
|
Spatial
resolution
|
collimator
with 1 degree FWHM
|
Detectors
|
5
proportional counters
|
Collecting
area
|
6500
square cm
|
Layers
|
1
Propane veto; 3 Xenon, each split into two; 1 Xenon veto layer
|
Sensitivity
|
0.1
mCrab
|
Background
|
2
mCrab
|
Events detected by the PCA will be processed on board by the EDS before
insertion into the telemetry stream.
Intrument built by CASS at UCSD which will study X-rays. HEXTE consists
of two clusters each containing four phoswich scintillation counters. The
clusters can rock at right angles to each other, with amplitudes of 1.5 or 3
degrees, to provide accurate background measurements. The total collecting area
is 1600 square cm. The instrumental properties are:
Energy
range
|
20
- 250 keV
|
Energy
resolution
|
&<
18% at 60 keV
|
Time
resolution
|
10
microsec
|
Spatial
resolution
|
collimator
with 1 degree FWHM
|
Detectors
|
2
times 4 scintillation counters
|
Collecting
area
|
1600
square cm
|
Phoswich
|
NaI
/ CsI
|
Sensitivity
|
10
mCrab
|
Background
|
100
mCrab
|
Events detected by HEXTE will be processed on board by its own data system
before insertion into the telemetry stream. It will allow event mode, histogram
binned mode, multiscalar mode, PHA/PSA spectral mode, and burst mode formats.
ASM, built by the CSR at MIT, will spot X-ray flare stars and burst
sources. It consists of three wide-angle shadow cameras equipped with
proportional counters with a total collecting area of 90 square cm. The
instrumental properties are:
Energy
range
|
2
- 10 keV
|
Time
resolution
|
80%
of the sky every 90 minutes
|
Spatial
resolution
|
3'
x 15'
|
Number
of shadow cameras
|
3,
each with 6 x 90 degrees FOV
|
Collecting
area
|
90
square cm
|
Detector
|
Xenon
proportional counter, position-sensitive
|
Sensitivity
|
30
mCrab
|
Events detected by the ASM will be processed on board by the EDS before
insertion into the telemetry stream.
The EDS consists of eight Event Analyzers (EA), of which two are
dedicated to the PCA and six to the ASM. Each EA contains an Intel 80286
processor and associated memory. The EAs can be programmed independently to
process incoming events from the instruments in any of the following modes:
Transparent mode, using 1, 2, or 3 EAs
Event mode, using 1 or 2 EAs
Binned mode (time and/or energy)
Burst catcher mode
Fourier transform mode
Pulsar fold mode
Autocorrelation mode
Arrival time differences histogram mode
It is being built by the CSR at MIT.
Telemetry: 2287.5 MHz (realtime: 16/32 kbps, playback: upto 1024
kbps)
Command: 2106.4 MHz (1/0.125 kbps)