FAST ComTec CSPA10 User Manual Download Page 3

CSPA1X_20210623 

Page 

1

FAST ComTec GmbH, Grünwalder Weg 28a, 82041 Oberhaching, phone: 49-(0)89 665180 -0, fax: 49-(0)89 665180 40, 

http://www.fastcomtec.com

 

   

                   

Description

FAST ComTec’s CSPA10...13 is a single channel charge 

sensitive preamplifier module intended for use with various 
types of radiation detectors including semiconductor 

detectors (e.g. CdTe and CZT), p-i-n photodiodes, 
avalanche photodiodes (APDs), and various gas-based 

detectors. 
The CSPA10 is one of a series of four charge sensitive 

preamplifiers offered by FAST ComTec, which differ from 
each other most notably by their gain. A guide to selecting 

the best charge sensitive preamplifier for your application 
can be found at our web site: http://www.fastcomtec.com. 

The CSPA1X is a successor model of CSP1X, with easier 
classic power supply. Other improvements include 

integrated protection circuits and better variability.

Equivalent circuit diagram

Figure 2 shows a simplified equivalent circuit diagram of the

CSPA10, which is a two stage amplifier. The first stage is 
high gain, and the second stage is low gain with an 

emphasis on supplying sufficient output current to drive a 
terminated coaxial cable. R

f

 (100 MΩ) and C

f

 (1.4 pF) are 

the feedback resistor and capacitor respectively (t

decay

140μs). The feedback values for the other models are:

R

f

 =10 MΩ and C

f

 =15 pF, t

decay

= 150μs (CSPA11),

R

f

 =680 kΩ and C

f

 =75 pF, t

decay

= 50μs (CSPA12),

R

f

 =68 kΩ and C

f

 =750 pF, t

decay

= 50μs (CSPA13).

Theory of operation

Charge sensitive preamplifiers are used when radiation is

detected as a series of pulses, resulting in brief bursts of
current flowing into or out of the preamplifier input. 

Depending on the type of detector, this burst of current may
be very brief (<1 ns) or as long as a few μs. For an 

idealized detection current pulse taking the form of a delta 
function, the detected charge (time integral of the input 

current) will ideally take the form of a step function. 
The output waveform of an actual charge sensitive 

preamplifier will of course have a non-zero rise time: for the
CSPA10 this figure is approximately 7 ns. Furthermore, 

capacitance at the preamplifier input (i.e. detector 
capacitance) will further slow the rise time at a rate of 

0.4 ns / pF. Keep in mind the output rise time will also be 
limited by the speed of the detector. For example, the 

detection current pulse from a CsI(Tl)/photodiode 
scintillation detector has a duration of approximately a 

couple μs, so the expected rise time of the charge sensitive 
preamplifier output will be at least that long. 

The output waveform of the CSP10 using a capacitively 
coupled fast square wave pulser at the input is shown below

to the left. At long time domains, the output decays due to 
the discharge of the feedback capacitor through the 

feedback resistor, with an RC time constant of 140 μs. This 
decay of the output waveform is also shown below, to the 

right.

CSPA1X charge sensitive preamplifier

Summary of Contents for CSPA10

Page 1: ...CSPA10 13 Charge Sensitive Preamplifier User Manual Copyright FAST ComTec GmbH Gr nwalder Weg 28a D 82041 Oberhaching Germany Version 1 05 July 15 2021 F ComTec GmbH 1...

Page 2: ...nsibility of the Costumer except for defects discovered within 30 days after receipt of equipment where shipping expense will be paid by FAST ComTec Copyright Information Copyright 2021 FAST ComTec Gm...

Page 3: ...80 k and Cf 75 pF tdecay 50 s CSPA12 Rf 68 k and Cf 750 pF tdecay 50 s CSPA13 Theory of operation Charge sensitive preamplifiers are used when radiation is detected as a series of pulses resulting in...

Page 4: ...Gain mV picoCoulomb Max detect Pulse e equiv noise in silicon keV FWHM CSPA10 1400 107 1 7 keV CSPA11 150 108 6 0 keV CSPA12 15 109 65 keV CSPA13 1 5 1010 230 keV Table 2 model specifications noise r...

Page 5: ...ion 11 4 1 Noise Consideration 11 4 2 Detector Bias 11 5 Operating Instructions 12 5 1 General 12 5 2 Test Input 12 5 3 Initial Setup 12 5 4 Initial Checkout 12 5 5 Protection Circuit 13 5 6 Common Op...

Page 6: ...nal Schematic diagram 7 Fig 3 1 Front and Rear panel 10 Fig 6 1 Simplified circuit diagram 16 Fig 7 1 CSPA1X board with jumpers 17 Fig 7 2 CSPA1X board with connectors 17 Fig 8 1 Detailed circuit diag...

Page 7: ...detector when the high voltage is applied Increase or decrease the high voltage only at a very slow rate Observe the output of the CSPA1X during bias voltage change with an oscilloscope Do not allow...

Page 8: ...ely biased SSB detectors the extremely linear energy output provides a negative polarity pulse ideal for energy spectroscopy The high charge rate capability of the design is evidenced by an energy rat...

Page 9: ...S CSPA11 2S Charge sensitive preamp SHV 2 kV 10 nF 150 mV pC CSPA112S CSPA12 2S Charge sensitive preamp SHV 2kV 10nF 15 mV pC CSPA122S CSPA13 2S Charge sensitive preamp SHV 2 kV 10 nF 1 5 mV pC CSPA13...

Page 10: ...page 2 CSPA10 Maximum charge detectable per event see table 1 Operating temperature 40 to 85 C Measured with input unconnected using Gaussian shaping amplifier with time constant 1 s With a detector a...

Page 11: ...NC for the models CSPA1x 1B Output BNC Test input BNC 2 5 Power Power supply voltage Vs 12 volts nominal ext 12V plug in power supply with 1 8m cable Power supply current 30 mA Power dissipation 400 m...

Page 12: ...controls and connectors located on the front and rear panels of the Model CSPA10 13 It is recommended that this section be read before proceeding with the operation of the preamplifier 3 2 Front Panel...

Page 13: ...the value of R reduced to provide a voltage drop The latter will cause the 0 pF noise of the preamplifier to increase but this will usually be insignificant compared to the noise generated in the det...

Page 14: ...tors This input does provide a resistive terminating impedance In the endless mode data acquisition is started only once e g by a software start i e asynchronously to the rest of the experiment Then a...

Page 15: ...ined are far different from what is expected it then becomes necessary to troubleshoot the system First observe the amplifier output on an oscilloscope at various time base and amplitude settings Is t...

Page 16: ...oad resistor dirty or moist detector input connector If RE and RD are acceptable but the live spectrum RS is not as good as expected the problem is probably in the detector bad detector poor charge co...

Page 17: ...ime of the charge sensitive preamplifier output will be at least that long The output waveform of the CSP10 13 using a capacitively coupled fast square wave pulser at the input is shown below to the l...

Page 18: ...Theory of Operation 16 F ComTec GmbH Fig 6 1 Simplified circuit diagram...

Page 19: ...otection network active 2 3 protection passive JP3 1 2 shorted inp ser resistor 0 Ohm 2 3 inp ser resistor 100 Ohm JP9 1 2 shorted output resistor 1 Ohm 2 3 output resistor 50 Ohm marked default setti...

Page 20: ...Appendix 8 Appendix 8 1 Detailed Schematic of the CSPA10 13 18 F ComTec GmbH Fig 8 1 Detailed circuit diagram of CSPA1X...

Page 21: ...Appendix 8 2 Personal Notes F ComTec GmbH 19...

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