ASTROSAT Charged Particle Monitor (CPM):
A charged particle monitor (CPM) will be included as a part of
ASTROSAT payloads to control the operation of the LAXPC, SXT and SSM.
Even though the orbital inclination of the satellite will be 8 deg
or less, in about 2/3rd of the orbits, the satellite will spend a
considerable time (15 - 20 minutes) in the South Atlantic Anomaly
(SAA) region which has high fluxes of low energy protons and
electrons. The high voltage will be lowered or put off using data
from CPM when the satellite enters the SAA region to prevent
damage to the detectors as well as to minimize ageing effect in
the Proportional Counters.
A Scintillator Photodiode Detector (SPD) with a Charge Sensitive
Preamplifier will be used to detect the charged particles.
In the ASTROSAT CPM, a
10 x 10 x 10 mm cube of CsI (Tl) crystal (wavelength = 550 nm)
with Teflon reflective material is coupled to the same area
window of a Si-PIN diode. The incident charged particle
energy is converted into light in CsI, and the light seen by the
photodiode is converted into an electrical pulse with the help of
a charge sensitive pre-amplifier (CSPA). The electrical signal is
then passed through a Lower Level Discriminator (LLD) with a
threshold level commandable from ground. The output is made
available to all other instruments on board, and is also recorded
as a part of the satellite housekeeping data.
Some salient features of the CPM are:
Scintillator |
: |
1cm x 1cm x 1cm CsI (Tl) crystal
|
Light collector |
: |
Photodiode with pre-amp
(Hamatmatsu s3590-08+eV5152) |
Window |
: |
1 mil Kapton |
Low energy threshold |
: |
1.2 MeV |
Time resolution |
: |
5 s |
Expected count rate |
: |
1 s-1 (non-SAA) |
Max. count rate |
: |
1000 s-1 |
Overall size |
: |
18cm x 15cm x 5cm |
Weight |
: |
2 kg |
Power requirement |
: |
2.3 W |