Development And Testing Of A Fast Fourier Transform High .

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REVIEW OF SCIENTIFIC INSTRUMENTS 80, 103504 共2009兲Development and testing of a fast Fourier transform high dynamic-rangespectral diagnostics for millimeter wave characterizationD. J. Thoen,1 W. A. Bongers,1 E. Westerhof,1 J. W. Oosterbeek,2 M. R. de Baar,1M. A. van den Berg,1 V. van Beveren,1 A. Bürger,2 A. P. H. Goede,1 M. F. Graswinckel,1B. A. Hennen,1,3 and F. C. Schüller11Association EURATOM-FOM, Trilateral Euregio Cluster, FOM-Institute for Plasma Physics Rijnhuizen,P.O. Box 1207, 3430 BE Nieuwegein, The Netherlands2Association EURATOM-FZJ, Institut für Energieforschung-Plasmaphysik, Forschungszentrum Jülich GMBH,52425 Jülich, Germany3Control Systems Technology Group, Eindhoven University of Technology, P.O. Box 513,NL-5600 MB Eindhoven, The Netherlands共Received 7 July 2009; accepted 15 September 2009; published online 21 October 2009兲A fast Fourier transform 共FFT兲 based wide range millimeter wave diagnostics for spectralcharacterization of scattered millimeter waves in plasmas has been successfully brought intooperation. The scattered millimeter waves are heterodyne downconverted and directly digitizedusing a fast analog-digital converter and a compact peripheral component interconnect computer.Frequency spectra are obtained by FFT in the time domain of the intermediate frequency signal. Thescattered millimeter waves are generated during high power electron cyclotron resonance heatingexperiments on the TEXTOR tokamak and demonstrate the performance of the diagnostics and, inparticular, the usability of direct digitizing and Fourier transformation of millimeter wave signals.The diagnostics is able to acquire 4 GHz wide spectra of signals in the range of 136–140 GHz. Therate of spectra is tunable and has been tested between 200 000 spectra/s with a frequency resolutionof 100 MHz and 120 spectra/s with a frequency resolution of 25 kHz. The respective dynamicranges are 52 and 88 dB. Major benefits of the new diagnostics are a tunable time and frequencyresolution due to postdetection, near-real time processing of the acquired data. This diagnostics hasa wider application in astrophysics, earth observation, plasma physics, and molecular spectroscopyfor the detection and analysis of millimeter wave radiation, providing high-resolution spectra at hightemporal resolution and large dynamic range. 2009 American Institute of Physics.关doi:10.1063/1.3244091兴I. INTRODUCTIONThe main route to the development of fusion power isthrough the tokamak device. In a tokamak, high temperatureplasma is confined by magnetic fields, which form nestedtoroidal magnetic flux surfaces,1 characterized by their magnetic winding number q. Performance limiting instabilities,such as the magnetohydrodynamic neoclassical tearing mode共NTM兲, occur at surfaces with simple rational q values suchas 2/1 and 3/2. These NTMs create magnetic islands throughthe breaking and reconnection of magnetic field lines on either side of the resonant surface, leading to a flattening of thepressure profile across the magnetic islands2 and hence a lossof plasma performance. Electron cyclotron heating and current drive 共ECH&CD兲 has demonstrated the ability to suppress NTMs on tokamaks.3–6ECH&CD and electron cyclotron emission 共ECE兲 takeplace at localized areas in the plasma where the wave frequency is resonant with the local electron cyclotron frequency or one of its harmonics. In current tokamaks thisfrequency is in the order of 100 GHz. At this frequency amillimeter wave beam propagates quasioptically as a Gaussian beam, which can be focused by mirrors, such that thepower is directed at a well-localized area in the plasma. Sup0034-6748/2009/80共10兲/103504/10/ 25.00pression of NTMs requires the precise deposition ofECH&CD at the center of the island 共O-point兲.On the TEXTOR tokamak, ECH&CD 共Refs. 7 and 8兲operates at 140 GHz produced by an 850 kW, 10 s pulselength gyrotron with steerable launcher.9 The installation features a pilot scheme for an in-line ECE feedback controlsystem,10–12 which is designed to detect the radial location ofthe island and the phase between O- and X-points 共islandtip兲. These measured ECE signals are used to control thesteering of the ECH&CD launcher in a feedback loop. Inline ECE refers to the ECE plasma signal being observedalong the same path traveled by the high power ECH&CDbeam, thus ensuring inherent positional accuracy. In TEXTOR tearing modes are generated in controlled fashion bymagnetic field perturbation coils, the so-called dynamic ergodic divertor 共DED兲.13During TEXTOR ECH&CD experiments an unexpectedly strong millimeter wave signal was observed,10 limitingthe operation of the in-line ECE receiver by saturating thedetector channels of the receiver. The nature of this spurioussignal is yet unknown and is shown to be no direct reflectionof ECH&CD waves from the plasma, but originating fromthe magnetic island O-point region.14 Trying to understandthe nature of the signal is important for two reasons. First,80, 103504-1 2009 American Institute of PhysicsDownloaded 25 Jan 2010 to 131.155.67.58. Redistribution subject to AIP license or copyright; see http://rsi.aip.org/rsi/copyright.jsp

103504-2Rev. Sci. Instrum. 80, 103504 共2009兲Thoen et al.detailed experimental data of millimeter wave scattering atthese frequencies constrains the theory of electron cyclotronwave propagation and absorption in high-pressure low collisional plasmas. Second, ECH&CD control of NTMs by thein-line ECE scheme requires physics understanding of theorigin in order to avoid disturbance of NTM control in largermachines such as ITER, which will operate at higher plasmatemperatures, lower collisionality, and higher ECH&CDpower.Investigation of the origin of the spurious signals requires measurements at high frequency resolution, high temporal resolution, and high dynamic range. Current in-lineECE and collective Thomson scattering15,16 共CTS兲 diagnostics on TEXTOR achieve a temporal resolution of up to 0.1MHz and a dynamic range of 26 dB. However, the totalfrequency range is limited by the number of channels and thefixed bandwidth of the detector channels. The in-line diagnostics has six spectral channels spaced 3 GHz with bandwidth of 500 MHz, the CTS covers 6 GHz with 42 spectralchannels, with bandwidths from 80 to 750 MHz. For detailedanalysis of the unknown signals, these frequency resolutionsare too low. Therefore a new dedicated diagnostics withhigher frequency resolution has to be developed, using directdigitizing and postdata acquisition signal processing basedon fast Fourier transform 共FFT兲 to make it possible to optimize time and frequency resolution.17This paper describes the design choices, implementation,and first operation of this new dedicated diagnostics. It hasthe following structure: Sec. II specifies the requirements ofthe diagnostics. Section III reviews the underlying theory.Section IV presents laboratory tests and selection of individual components and also measurements and calculationsto characterize and calibrate the integrated system. Section Vdemonstrates the performance of the new diagnostics in scattering measurements on TEXTOR. Section VI discusses theresults and proposes recommendations for future work. Section VII concludes the paper.II. REQUIREMENTSat varying DED phase. This increases the frequency resolution under the assumption that the bursts repeat exactly.The minimum time resolution for the diagnostic is set bythe requirement to resolve a single spike at a typical DEDfixed island rotation frequency. This leads to a temporal requirement of 5 s, with 40 frequency bands of 100 MHzwidth. The aliasing allows for longer time scales of 0.1 msand hence 16 000 bands of 0.25 MHz width. The system willthus be able to acquire 10 000 waveforms/s with ⱕ8000samples and 200 000 waveforms/s with ⱕ80 samples. Toallow for a variable frequency and time resolution the systemmust be based on a digitizer.No diagnostics exists for direct measurement of signalsin the 100 GHz frequency range. The common approach is todownconvert the frequency by means of heterodyne mixing,yielding a frequency range of 0–4 GHz. When digitizing thissignal, according to the Nyquist criterion, a sampling frequency of at least 8 GHz is required in order to avoid loss ofinformation due to aliasing.19 The choice of heterodyne detection with digitizing sets constraints on the amplificationand the noise figure 共NF兲. Requirements derive from thedigitizer selected. To allow for simultaneous ECE and scattering measurements, the dynamic range of the instrumentshould exceed 40 dB. The signal to noise ratio 共SNR兲 requirement is set at 40 dB.The above requirements refer to the sampling of data foroff-line processing and analysis. Future development includes a FFT based ECE feedback control system,20 whichrequires a data handling capacity in excess of 5 GSa/s. It isnoted that diagnostics with the above characteristics can beapplied to other fields of science, such as earth observation,astrophysics, molecular spectroscopy using millimeter waveobservations for understanding atmospheric composition, interstellar clouds, and molecular line shapes.B. Requirements flow downRequirements of individual elements of the detectionchain follow from the top-level functional requirements.Some requirements are based on limits that can be practicallyachieved.A. Top level requirementsThe spurious scatter signal to be investigated appears inperiodic bursts occurring on the typical time scale of plasmarotation 共millisecond兲 with a signal frequency ranging from136 to 140 GHz. Each burst displays a strong amplitudevariation 共spikes兲 on a submillisecond time scale. CTS measurements show that the events have a radiation temperatureof 100 keV.18 Characterization of the signal requires thesimultaneous measurement by CTS and ECE diagnostics.From CTS measurements the bursts of spurious signals appear to have their origin inside the O-point of the islands andare therefore synchronized with the rotation of the islands.The tearing mode is induced in TEXTOR plasma by theDED and therefore accurately controlled by the DED in frequency and phase. This allows two basic approaches for diagnosis: The first is to resolve a single spike at moderatefrequency resolution. Alternatively, by deliberately aliasing,a spike can be reconstructed from a number of spike samples1. Heterodyne front endA heterodyne receiver mixes the radio frequency 共rf兲 signal with frequency f rf with a local oscillator 共LO兲 frequencyf LO to downconvert to an intermediate frequency 共IF兲signal.21 The process of mixing is mathematically equivalentto multiplying two harmonics yielding up- and downconverted frequency difference components. In this case, the f rfrange is between 136 and 140 GHz. Fixing f LO at 140 GHzyields an IF band between 0 and 4 GHz. This refers to thesignal downconverted to the lower sideband. However, signals ranging from 140 to 144 GHz at the upper sideband arealso generated. The CTS measurements showed signals between 137 and 140 GHz, indicating no sideband filtering isrequired. A benefit is the improved SNR behavior withoutfiltering. Amplification is needed to ensure compatibilitywith the input level of the digitizer. An added benefit ofDownloaded 25 Jan 2010 to 131.155.67.58. 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103504-3Rev. Sci. Instrum. 80, 103504 共2009兲Thoen et al.sufficient amplification is that the noise in the system approaches the theoretical noise temperature limit.2. MixerMixers are characterized by rf and IF ranges, conversionloss, and NF. The requirements on the mixer are rf range of 136–140 GHz, conversion loss of 20 dB, and NF of 20 dB.The latter two requirements flow down from the top-levelrequirement of simultaneous measurement of ECE and scattered signal. Ideally, the IF range extends from direct current共dc兲 to 4.0 GHz, but this is no strict requirement. The outputof the mixer has a 4 GHz bandwidth and is sampled at 8GHz. To avoid aliasing of high 共 4 GHz兲 frequency components, the mixer output signals can be filtered.3. Local oscillatorThe requirements on the LO are frequency stability of 140.00 GHz 0.01 GHz and LO output power matches rf input power of the mixer, viz., 10 mW.TS T1 T2T3 ,G 1 G 1G 2共1兲where the equivalent noise temperatures Tn can be calculatedfrom the noise factor F and the ambient temperature T0 : Tn 共F 1兲T0. The gain Gn is considered a loss when Gn issmaller than unity. Expressed in decibels as NF 10 log F,the noise factor is called NF, which will be used throughoutthis report.The total equivalent noise temperature Ttot of an ECEsystem in a tokamak is the sum of the noise temperature ofthe plasma electrons 共Te兲 and the noise temperature of theECE diagnostics:24 Ttot Te TS. Ideally, the thermal noise ofthe electrons is dominating over all other noise sources. Tsfor our system is calculated by using a derived cascade noiseequation: TS 共Lwg 1兲T0 LwgTR, where Lwg is the loss in thetransmission line in decibel and TR is the equivalent noisetemperature of the radiometer. Combining these equationsyieldsTtot Te 共Lwg 1兲T0 LwgTR .共2兲The total noise temperature serves to estimate the minimumdetectable power.21B. FFT, SNR, and sensitivity4. AmplifierAmplifiers are characterized by their bandwidth, gain,NF, and dynamic range. Requirements on the amplifier are frequency range dc 4 GHz;gain of 30 dB,low noise characteristics, NF 5 dB, andmaximum output power level of 10 dBm.The requirement on the NF flows down from the requirementof simultaneously measure ECE and scattered signal.The gain of the amplifier must match to a full scalereading of the digitizer. For fixed gain amplifiers the inputpower level should not exceed the maximum input powerlevel of the digitizer minus the amplifier gain.5. DigitizerRequirements on the digitizer are signal sampling frequency of 8 GHz, a tunable retrigger rate of 10–200 kHz, data storage sufficient to store 1.0 s of data, equivalentto 16 106 samples, and output dataflow of 100 MSa/ s to allow for FFT basedECE feedback control.III. THEORYA. NoiseThe 共equivalent兲 noise temperature of a system 共Ts兲 canbe calculated using the cascade noise equation of Friis,21–23The spectral resolution f of a FFT is a function of thesample rate f s of the analog-digital converter 共ADC兲 and thenumber of time domain samples N,19 f fs.N共3兲For a given sample rate, increasing the number of samplesincreases the frequency resolution.When using FFT, spectral leakage will occur.19 Spectralleakage can be limited by applying windows on the timedomain signal. Several shapes of windows are available, ofwhich the flattop window is best suited for relatively wideband signals, providing increased amplitude accuracy.17,25The number of samples in the frequency domain can becalculated from the time domain sample size,N f 21 N 1.共4兲Throughout this report the number of samples referred to isthe time domain sample size N unless stated otherwise.For classical radiometers, their sensitivity can be obtained from the radiometer formula21,24,26冑Pmin kBBTtot2Bvid,BIF共5兲with Pmin as the least detectable power 共W兲, kb as Boltzmann’s constant, 1.38 10 23 W / K, B as the input bandwidth 共Hz兲, Ttot as the total equivalent noise temperature ofthe system 共K兲, Bvid as the video bandwidth of the radiometer共Hz兲, and BIF as the IF bandwidth of the radiometer 共Hz兲.Combining Eqs. 共3兲 and 共5兲 and the expression for the bandwidth and taking B BIF yieldsDownloaded 25 Jan 2010 to 131.155.67.58. Redistribution subject to AIP license or copyright; see http://rsi.aip.org/rsi/copyright.jsp

103504-4Rev. Sci. Instrum. 80, 103504 共2009兲Thoen et al.冑Pmin kB f sTtotTABLE I. High-speed data acquisition systems examined.1N共6兲expressing the minimal detectable power of a FFT basedreceiver.The SNR of an ideal digitizer with Nb bits can be calculated following Bennett,19 showing that the full scale sinewave SNR is given bySNR 6.02Nb 1.76 dB 10 logfs,2 fModelTypeAgilentESA E4407BSpectrum analyzerTektronixRSA 6100, Opt.110RT spectrum analyzerAgilentDSO 90804A InfiniiumOscilloscopeTektronixDPO 70000 seriesOscilloscopeAgilent/AcqirisDC-222cPCI card system/digitizerNational InstrumentsNI-PXI 5663PXI card system/digitizer共7兲where the latter part is the process gain. Substituting Eq. 共3兲in Eq. 共7兲 yieldsNSNR 6.02Nb 1.76 dB 10 log .2Manufacturer共8兲This is the FFT noise floor of an 共ideal兲 ADC. When theSNR of the ADC is known, the effective number of bits Nb共ENOB兲 of the ADC can be calculated.IV. TESTINGA. Heterodyne mixingTwo mixers have been tested: A mixer manufacturedby AI-ATD Division, series 041, model 9602 marked F0 140 GHz, which is a double sideband mixer; a mixermanufactured by Millitech MWW Division, type MXF-06ES, which is custom made for the Rijnhuizen tokamakproject and is designed for a LO of 128 GHz and optimizedfor an IF of 6–18 GHz. The mixer is single ended. Thismeans the LO has to be combined with the rf signal beforeentering the mixer. This process is done by an external 10dB coupler.The average conversion loss of the AI-ATD mixer is 33 dB. The conversion loss of the Millitech mixer has anaverage value of 15 dB.The NF of the AI-ATD mixer is unknown, although it isreasonable to assume that it is equal to the conversion loss atmaximum, resulting in a NF 35 dB. The NF of the Millitech mixer is 10 dB according to the manufacturer.a maximum input power of 13 dBm. The WENTEQamplifier has a gain of 35 dB and NF 4.6 dB. The P 1 dB 14 dBm, giving a maximum input power level of 18dBm. The gain and NF performance of the WENTEQ amplifier are better than that of the MINI-CIRCUITS device, making it the best suited device for the rf front end.C. High-speed data acquisitionThe choice of the digitizer is based on the requirementsstated in Sec. II with bandwidth requirement of 4 GHz orover. Six digitizers have been examined in order to find thebest fit to the requirements: two spectrum analyzers, twomemory scopes, and two high speed data-acquisition cardsystems 共see Table I兲. Table II lists the performance of thevarious types of digitizer.1. Trigger rateThe retrigger rate is the time required for the system tobe able to receive another 共series兲 of triggers, in order to docontinued measurements. The oscilloscopes are able to acquire up to 300 000 waveforms/s but their retriggering of thesystem is limited to the screen refreshment rate of 50 Hz.All except the spectrum analyzer are capable of retrieving data at the required trigger rate. According to the specifications the Agilent spectrum analyzer is not capable of retrieving more than about 40 triggers/s.2. BandwidthB. AmplificationTwo amplifiers have been examined. The MINICIRCUITS amplifier has a gain of 30 dB and a NF of 6 dB.The maximum output level is P 1 dB 17 dBm, resulting inThe requirement on the real time 共RT兲 bandwidth is 4GHz. The tested spectrum analyzer and both oscilloscopeshave wider bandwidths of 26.5 and 8 GHz, respectively. Tektronix RTSA has a RT bandwidth of 110 MHz. The band-TABLE II. Trade-off matrix indicates the performance of the various types of digitizers. The cPCI system ofAcqiris meets or exceeds all requirements. Digitizer performance is indicated per channel, if applicable.DigitizerRequirementsAgilent SATektronix RTSAAgilent scopeTektronix scopeAcqiris cPCINI PXITrigger rate共kHz兲Retrigger rate共kHz兲RT bandwidth共GHz兲Data flow共MSa/s兲2004 10 25 1043003001063002004 10 26 1045 10 25 10 21060.3426.50.1102.5–134–204.00.05100 0.01Unknown, but RT2210 20075Downloaded 25 Jan 2010 to 131.155.67.58. Redistribution subject to AIP license or copyright; see http://rsi.aip.org/rsi/copyright.jsp

103504-5Rev. Sci. Instrum. 80, 103504 共2009兲Thoen et al.FIG. 1. 共Color online兲 Noise floor of the frequency measurement system without signal input. The ADC’s maximum input power of 4 dBm is normalizedat 0 dB. The measurements are in g

Electron cyclotron heating and cur-rent drive ECH&CD magnetic field perturbation coils, the so-called dynamic er-has demonstrated the ability to sup-press NTMs on tokamaks.3–6 ECH&CD and electron cyclotron emission ECE take place at localized areas in the plasma where the wave fre-quency is resonan

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