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Far-Infrared THz FTIRMain Features:
For some information about latest measurements made by renowed world scientists in TeraHertz sciences click: http://www.kbfi.ee/thz/?p=spssoftware SPS-300 System The base system of the SPS-300 includes: SPS-300 Body consisting of:
Additional requirements for Spectral Analyzer configuration: Detector and light input port with flipping mirror Additional requirements for Materials Spectrometer configuration: Sample chamber and detector SKU: SPS-300 Sciencetech’s SPS-300 is a modular polarizing Fourier Transform Interferometer (FTS or FTIR) designed specifically to operate in the far-infrared and THz spectral region (5μm-5mm or frequency between 0.1-15 THz or in the band of 3-500cm-1). The modularity of the SPS-300 allows it to be configured as a far-infrared/THz light source spectral analyzer or as a materials transmission and reflectance spectrometer. The SPS-300 has large 90mm optics and can be operated in both classical Michelson mode with an aluminized Mylar beam splitter, and in Martin-Puplett Mode with a 5" diameter grid polarizer beam splitter that provides the broadest possible spectral range and makes the SPS-300 truly unique. The Polarizing mode also has other advantages in spectroscopy, biophysics, surface science, electrochemistry, material science, and infrared ellipsometry. For more information download the full FTIR brochure below. Technical Specifications Spectral Range: 2-2000cm-1 (5µm-5mm) Standard Resolution: 0.119cm-1 with 5cm translation stage High Resolution: 0.020cm-1 with 30cm translation stage Signal-to-Noise Ratio: varies with the source and detector selected, but with a standard Sciencetech detector and the built-in source, typical values are as follows: in Michelson mode: 0.4% in Martin-Puplett mode: 2.2% Optics: Martin-Puplett optical configuration, large 90mm optics, fast f/2.35 off-axis paraboloid condensers for high light throughput Grid Polarizer Beam Splitter: 2μm lines with 4μm pitch aluminum on Mylar substrate Body: vacuum steel housing capable of maintaining 10-3Torr Source: internal 75W Hg arc lamp (water cooled) with external DC stabilized power supply and igniter Controls: motorized roof mirror alignment (tilt, rotary shear, lateral shear) to fine tune interference at the beam splitter Ports: vacuum purge port, thermocouple vacuum gauge with analog dial display, inlet and outlet ports for water cooling of internal light source and stepper motors Scan: Step and Scan Mode (standard): detector data collection is synchronized with the translating roof mirror positioning. The mirror is moved to selected positions and readings are taken. Rapid Scan Mode: the roof mirror moves continuously and does not stop as detector collects data. Dimensions: 99 x 63 x 3cm (39”x 25”x15”) Weight: steel body: 180kg (397lb) stainless steel body 80kg (176lb). Pulsed Source operation
The SPS300 Pulsed mode upgrade allows the user operate with pulsed sources. In pulsed mode the mirror positioning and detector sampling are synchronized with pulses from the source. For pulse repetition rates greater than a couple of kHz the source can be considered as effectively continuous - i.e. normal CW operation can be used. However for lower rates synchronization prevents degradation of S:N due to sampling effects. The upgrade includes a TTL input for electrical synchronizing pulses.
Note that low pulse repetition rates require correspondingly long measurement times, as only a single step can be measured for each pulse.
Using the SPS-300, and either the standard bolometer we supply having NEP ~1.E-13 or the DTGS detector having NEP ~7.E-11, and considering 1nJ pulses, we estimate single pulse S/N ratios as follows : (not considering system losses)
Pulse rate: 10/s 1/s
Bolometer 30000:1 10000:1
DTGS 40:1 15:1
If source stability is poorer than the detector noise levels the pulse noise will dominate, but by using a second reference detector the S/N ratio in the interferogram can be improved toward the limit set by detector noise.
Price: $143,610.00 ( categories: )
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