There are a
number of considerations and trade-offs to make when
choosing the right charge sensitive preamplifier (CSP) for your application.
This guide will help to give you make the best decision.
It should be
made clear that all of Cremat's preamplifier models are
intended for use in radiation detection applications
where the radiation is detected as a series of pulses.
An example of this would be a gamma-ray spectrometer.
In this case, the detection of each gamma-ray produces an electronic
pulse that is amplified and measured. There are some radiation detection applications where
this is not the case. For example, in CT imaging X-ray
flux is detected as a time varying current, and the
detectors are read by transimpedance amplifiers.
Cremat's
preamplifier model having the highest gain and best noise performance is the CR-110, and
for this reason it may be the best choice for many
customers. There are a number of other considerations,
however, which may lead the user to choose one of the
three other preamplifier models. These considerations are
listed below:
1)
Maximum detectable pulse
In choosing
a preamplifier for your application, it is often best to
start by considering the model having the highest gain:
the CR-110. A potential problem, however, is that the
high gain of the CR-110 will cause large signal pulses
(larger than approximately 107 electrons) to
saturate the preamplifier circuitry. In these
applications it is best to choose a less sensitive
preamplifier. The gain, maximum detectable pulse
magnitude, and noise level of Cremat's preamplifier models are listed
here:
|
preamp
model |
gain (mV per
picoCoulomb) |
maximum detectable
pulse (electrons) |
noise (ENC) in electrons RMS* |
|
CR-110 |
1400 |
107 |
200 |
|
CR-111 |
150 |
108 |
630 |
|
CR-112 |
15 |
109 |
6,800 |
|
CR-113 |
1.5 |
1010 |
24,000 |
*
@1us shaping time, input
unconnected
A good
approach to selecting the
right preamplifier is to choose the model having the largest gain
which is also
capable of detecting the largest pulses you expect to
detect in your application.
If you are
unsure about how to calculate the size of the pulses in
your application, help may be found here:
Pulse size
calculation.
2)
Stability at high input
capacitance
In
applications where the input capacitance to the
preamplifier exceeds 2000 pF, the CR-110 becomes unstable
and may oscillate. In these rare applications users
should avoid using the CR-110 and instead select one of the
other preamplifier models, all of which are stable at high input
capacitance.
3) Rise-time
performance
The rise
time performance of Cremat's charge sensitive
preamplifiers (CSPs) vary amongst the various models, as
can be seen in the following table, where Cin
is the capacitance (in pF) at the preamplifier input:
|
preamp
model |
rise time (ns) |
|
CR-110 |
0.4·Cin
+ 7 ns |
|
CR-111 |
0.1·Cin
+ 3 ns |
|
CR-112 |
0.25·Cin
+ 6 ns |
|
CR-113 |
0.25·Cin
+ 20 ns |
Keep in mind
that in some detectors,
rise time will be limited by the detector itself. In these
cases the use of a faster preamplifier will not improve
the situation. In applications with fast detectors,
however, you may wish to choose your preamplifier with
these preamplifier rise time specifications taken into
consideration.
4) High
count rate
In high
count rate applications, the preamplifier circuitry can
sometimes saturate due to the high rate of detector
current being sourced or sunk at the preamplifier input. In
these high-rate applications, you may
wish to avoid the high gain preamplifier models (e.g.
CR-110) which are the most prone to this saturation.
Calculating
whether a particular preamplifier can process a certain
count rate is complicated, because the answer depends on
the distribution of pulse sizes being detected and the
distribution of events over time (e.g. random over time,
occurring only during certain time windows, etc). A
somewhat simplified approach would be to assume that the
pulses occur totally randomly over time and that the
detected pulses are very many small pulses (rather than
a few number of larger sized pulses).
If we assume
that the preamplifiers are DC coupled to the detector,
then we can treat the simplified detector current
described above as a DC current passing into the
preamplifier input. The maximum DC current that can be
sourced or sunk by Cremat's preamplifiers before
reaching saturation are given by the following table:
|
preamp
model |
maximum DC
input current (uA) |
|
CR-110 |
0.01 |
|
CR-111 |
0.1 |
|
CR-112 |
3 |
|
CR-113 |
30 |
In this
simplified case, the maximum count rate the preamplifier
would be able to process would be that which produced a
detector current equal to the maximum DC input current
listed in the above table. Note that the high gain
preamplifiers have the worst count rate processing
ability. Also consider that our assumption that the
detector current is comprised of many small pulses
represents a best-case condition for the preamplifier
maximum count rate.
If AC
coupling is used between the detector and preamplifier,
the count rate capability of the preamplifier is
dramatically increased, at least if we use our
simplifying assumption that the detector signal current
is made of very many small pulses. Using AC coupling,
the DC detector current no longer passes into the
preamplifier input. As a result, the preamplifier output
saturates only when the output fluctuations
become so large that they exceed the rail-to-rail output
range of the preamplifier (approximately 6 volts). The
size of these fluctuations depend on the size
distribution and rate of the detected pulses, and it is
difficult to quantitatively described the count rate
limitations of the preamplifiers under these conditions.
It remains true, however, that the highest gain
preamplifiers have the worst count rate processing
ability and the lowest gain the best.