The X-123SDD represents the culmination of years of electronics and X-ray detector innovation and development at Amptek. We remain focused on creating small, low power, high performance instruments while keeping them simple to operate. The X-123SDD epitomizes this philosophy by providing in a single package the XR-100SDD Silicon Drift X-Ray Detector and its Charge Sensitive Preamplifier; the DP5 Digital Pulse Processor (DPP) with pulse shaper, MCA, and interface; and the PC5 Power Supply. All that is needed is a +5 Volts DC input and a USB, RS-232 or Ethernet connection to your computer.
The X-123SDD combines Amptek’s high performance X-ray spectroscopy components in a single package:
The result is an extremely compact system with no performance compromise. It requires only +5 VDC power and a standard communication interface. With the X-123SDD and an X-ray source, anyone can rapidly obtain high quality X-ray spectra.Contact Us for more information today!
The X-123SDD uses a silicon drift detector (SDD) similar to a Si-PIN photodiode but with a unique electrode structure to improve energy resolution and increase count rates. The SDD is mounted on a thermoelectric cooler along with the input FET and coupled to a custom charge sensitive preamplifier. The thermoelectric cooler reduces the electronic noise in the detector and preamplifier but the cooling is transparent to the user: it operates like a room temperature system.
The pulse processor is the DP5, a second generation digital pulse processor (DPP) which replaces both the shaping amplifier and MCA found in analog systems. The digital technology improves several key parameters:
The DPP digitizes the preamplifier output, applies real-time digital processing to the signal, detects the peak amplitude, and bins this in its histogram memory. The spectrum is then transmitted to the user’s computer. The PC5 supplies the power to the detector, including low voltages for the preamps, high voltage to bias the detector, and a supply for the thermoelectric cooler which provides closed loop control with a maximum temperature differential of 85 °C. All of these are under software control. The X-123SDD input power is an unregulated +5 VDC with a current of about 300 mA.
The complete system is packaged in 7 x 10 x 2.5 cm3 aluminum box. The detector is mounted on an extender, with lengths from 0 to 9” (vacuum flanges are available). In its standard configuration only two connections are required: power (+5 VDC) and communications (USB, RS232, or Ethernet). An auxiliary connector provides several additional inputs and outputs used if the X-123SDD will be integrated with other equipment. This includes an MCA gate, timing outputs, and eight SCA outputs. The X-123SDD is supplied with our DPPMCA data acquisition and control software. It also includes an Application Programming Interface (API) DLL to integrate the unit with custom software. Options include software for analyzing X-ray spectra, vacuum accessories, several collimation and mounting options, and X-ray tubes to complete a compact system for X-ray fluorescence.
Figure 2. Resolution vs. Peaking Time and Temperature for the silicon drift detector (SDD).
Figure 4. Resolution vs. Input Count Rate for different peaking times for the silicon drift detector (SDD) with the DP5.
The plot also shows the curve of maximum output count rate. Operating to the right of that curve results in less throughput than the maximum despite a higher input rate. See figure 5 below.
Figure 5. Throughput with the silicon drift detector (SDD). Due to the detector’s smaller capacitance, a much shorter peaking time is used in the shaping amplifier without sacrificing resolution. Typically 9.6 µs or less is used. This dramatically increases the throughput of the system.
In the bottom plot, the black curve represents “Fano broadening”, the theoretical limit with a Si based detectors, arising from quantum fluctuations in the charge production process. The colored curves represent the combination of Fano broadening and intrinsic electronic noise under optimum conditions (full cooling and long peaking time). The detector selection is most important at the lowest energies because Fano broadening dominates at high enough energies.
In the top plot, the efficiency at low energies is determined by transmission through the window and detector dead layer. The efficiency at high energies is determined by attenuation in the active depth of the detector. A Si detector with Be window is recommended between about 2 and 30 keV. A Si detector with a C1 or C2 window is recommended at lower energies, while a CdTe detector is best at energies above 30 keV
Efficiency Package: A ZIP file of coefficients and a FAQ about efficiency. This package is provided for general information. It should not be used as a basis for critical quantitative analysis.
|Energy Resolution||125 to 140 eV FWHM @ 5.9 keV. Depends on peaking time and temperature.|
|Electronic Noise (typical)||73 eV FWHM (8.7 e– rms)|
|Peak to Background||20,000:1 (ratio of counts from 5.9 keV to 1 keV) (typical)|
|Energy Range||Efficiency >25% for X-rays from 1 to 25 keV. May be used outside this range with lower efficiency.|
|Maximum Count Rate||Depends on peaking time. Recommended maxima with pile-up-rejection enabled are shown below.
|Detector Type||Silicon Drift Diode (SDD)|
|Detector Area||25 mm2 (collimator area 17 mm2)|
|Detector Thickness||500 µm|
|Detector Window Options||Beryllium (Be): 0.5 mil (12.5 µm) or 0.3 mil (8 µm)
Patented C-Series: C1 and C2 Low energy windows available with FAST SDD®
|Thermoelectric Cooler||2-stage (85° ΔTmax)|
|Preamplifier Type||Amptek custom reset, charge sensitive.|
|Preamp Conversion Gain||0.8 mV/keV (typical)|
|Gain||Combination of coarse and fine gain yields overall gain continuously adjustable from 0.84 to 127.5.|
|Coarse Gain||Software selectable from 1.12 to 102 in 16 log steps.
1.12, 2.49, 3.78, 5.26, 6.56, 8.39, 10.10, 11.31,
14.56, 17.77, 22.42, 30.83, 38.18, 47.47, 66.26, 102.0
|Fine Gain||Software selectable, 0.75 to 1.25, 10 bit resolution.|
|Full Scale||1000 mV input pulse @ X1 gain|
|Gain Stability||<20 ppm/°C (typical)|
|Pulse Shape||Trapezoidal (A semi-Gaussian amplifier with shaping time t has a peaking time of 2.2t and is comparable in performance with the trapezoidal shape of the same peaking time.)|
|ADC Clock Rate||20 or 80 MHz, 12 bit ADC|
|Peaking Time||30 software selectable peaking times between 0.2 and 102 µs, corresponding to semi-Gaussian shaping times of 0.1 to 45 µs.|
|Flat Top||16 software selectable values for each peaking time (depends on the peaking time), >0.05 µs.|
|Baseline Restoration||Asymmetric, 16 software selectable slew rate settings.|
|Fast Channel Pulse Pair Resolving Time||120 ns|
|Dead Time Per Pulse||1.05 times the peaking time. No conversion time.|
|Maximum Count Rate||4 x 106 s-1 (periodic). Output count rate of 7 x 105 s-1 for a random input of 1.9 x 106 s-1.|
|Dead Time Correction||Manual correction based on Fast Channel measurement of ICR. Accurate to 1% for ICR <1 Mcps under typical conditions.|
|Pulse Selection Options||Pile-up rejection, risetime discrimination, gate|
|Number of Channels||Software selectable to: 8k, 4k, 2k, 1k, 0.5k, or 0.25k channels|
|Bytes per channel||3 bytes (24 bits) – 16.7M counts|
|Acquisition Time||10 ms to 466 days|
|Data Transfer Time||1k channels in 12 ms (USB) or 280 ms (RS-232)|
|Presets||Time, total counts, counts in an ROI, counts in a single channel|
|MCS Timebase||10 ms/channel to 300 s/channel|
|External MCA Controls||Gate input: Pulses accepted only when gated on by external logic. Input can be active high or active low. Software controlled.|
|Counters||Slow channel events accepted by MCA, Incoming counts (fast channel counts above threshold), SCA8 counts, event rejected by selection logic, and external event counter. Sixteen ROI counters.|
|Single Channel Analyzers||8 SCAs, independent software selectable LLDs and ULDs, LVCMOS (3.3 V) level (TTL compatible)|
|Digital Outputs||Two independent outputs, software selectable between 8 settings including INCOMING_COUNT, PILEUP, MCS_TIMEBASE, etc. LVCMOS (3.3 V) levels (TTL compatible).|
|Digital Inputs||Two independent inputs, software selectable for MCA_GATE, EXTERNAL_COUNTER|
|I/O||Two general purpose I/O lines for custom application|
|Digital Oscilloscope||Displays oscilloscope traces on the computer. Software selectable to show shaped output, ADC input, etc., to assist in debugging or optimizing configurations.|
|USB||2.0 full speed (12 Mbps)|
|Serial||Standard RS-232 at 115.2k or 57.6k baud|
|Nominal Input Power||+5 VDC at 500 mA (2.5 W) (typical). Current depends strongly on detector ΔT. Ranges from 300 to 800 mA at 5 VDC.|
|Input Range||4 V to 5.5 V (at 0.4 to 0.7 A typical)|
|Initial transient||2 A for <100 µs|
|High Voltage Supply||Internal multiplier, software control -70 to -200 V, negative polarity|
|Cooler Supply||Closed loop controller with ΔTmax = 85 °C|
|Dimensions||7 x 10 x 2.5 cm (2.7 x 3.9 x 1 in) excluding extender|
|Extender Lengths||1.5” (3.8 cm) standard. Options include no extender, 3/8”, 5”, 9”, and vacuum flanges.|
|Weight||180 g (6.3 oz)|
|Operating temperature||-35 °C to +80 °C|
|Warranty Period||1 Year|
|Typical Device Lifetime||5 to 10 years, depending on use|
|Storage and Shipping||Long term storage: 10+ years in dry environment
Typical Storage and Shipping: -40 °C to +85 °C, 10 to 90% humidity noncondensing
Certificate #: CU 72101153 01
Tested to: UL 61010-1: 2009 R10.08
|USB||Standard USB ‘mini-B’ jack. (The X-123SDD does not draw power from the USB.)|
|RS232||Standard 2.5 mm stereo audio jack.
|Ethernet||Standard Ethernet connector (RJ-45)|
|Power||Hirose MQ172-3PA(55), Mating plug: MQ172-3SA-CV|
|Auxiliary||2 x 8 16-pin 2 mm spacing (Samtec part number ASP-135096-01). Mates with cable assembly (Samtec P/N TCMD-08-S-XX.XX-01. Top row odd pins, bottom row even pins. Top right pin = 1, bottom right pin = 2.
|DPPMCA||The X-123SDD can be controlled by the Amptek DPPMCA display and acquisition software. This software completely controls and configures the X-123SDD, and downloads and displays the data. It and supports regions of interest (ROI), calibrations, peak searching, and so on. The DPPMCA software includes a seamless interface to the XRF-FP quantitative X-ray analysis software package. Runs under Windows XP PRO SP3 or later. Click here for the software download page.|
|SDK||The X-123SDD comes with a free Software Developer’s Kit (SDK). The user can use this kit to easily write custom code to control the X-123SDD for custom applications or to interface it to a larger system. Examples are provided in VB, VC++, etc. Click here for the software download page.|
|VB Demonstration Software||The VB demonstration software runs on a personal computer and permits the user to set the X-123SDD parameters, to start and stop data acquisition, and to save data files. It is provided with source code and can be modified by the user. This software is intended as an example of how to manually control the X-123SDD through either the USB, RS-232, or Ethernet interface using the most basic calls without the SDK. This is primarily needed as an example when writing software for non-Windows platforms. Click here for the software download page.|
Figure 9. XRF of stainless steel SS316 taken with the silicon drift detector (SDD) and the Mini-X x-ray tube.
Amptek SDDs are available with beryllium windows, and our FastSDDs are optionally available with our C-Series windows. The Be options are Paralyne coated (to prevent gas diffusion), and are supplied in two thicknesses, 0.3 mil or 0.5 mil (8 or 12.5 μm). The Patented C-Series windows are designed for low Z element detection down to Boron (B).
Figure 15a. The XR100SDD/PX5 configuration, which includes the detector, preamplifier, digital processor, and power supplies.
Figure 15b. The detector/preamplifier is available in OEM configurations to fit the requirements of any system. Pictured is the detector with the PA-230 preamplifier and housing. See the OEM page for details.
All of Amptek’s Si detectors contain internal multilayer collimators to improve spectral quality. X-rays interacting near the edges of the active volume of the detector may produce small pulses due to partial charge collection. These pulses result in artifacts in the spectrum which, for some applications, obscure the signal of interest. The internal collimator restricts X-rays to the active volume, where clean signals are produced. Depending on the type of detector, collimators can improve peak to background (P/B), eliminate edge effects, eliminate false peaks.
A multilayer collimator is made by progressively using lower Z materials. Each layer acts as an absorber to the fluorescence peaks of the previous layer. The final layer will be of the lowest Z material whose fluorescence peaks are of low enough energy to be outside the anticipated X-ray detection range.
Amptek has developed a state-of-the-art internal Multilayer Collimator (ML). The base metal is 100 µm of tungsten (W), the first layer is 35 µm of chromium (Cr), the second layer is 15 µm of titanium (Ti), and the last layer is 75 µm of aluminum (Al).
Download the X-123 STP File
All results on this page are typical performance values at full cooling; please Contact Us to discuss guaranteed performance under different operating conditions. Specifications subject to change without notice.