ITU-R SM 1754-2006 Measurement techniques of ultra-wideband transmissions (Question ITU-R 227 1)《超宽带传输测量技术 问题ITU-R 227 1》.pdf

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1、 Rec. ITU-R SM.1754 1 RECOMMENDATION ITU-R SM.1754 Measurement techniques of ultra-wideband transmissions (Question ITU-R 227/1) (2006) Scope Taking into account that there are two general measurement approaches (time domain and frequency domain) this Recommendation gives the appropriate techniques

2、to be applied when measuring UWB transmissions. The ITU Radiocommunication Assembly, considering a) that intentional transmissions from devices using ultra-wideband (UWB) technology may extend over a very large frequency range; b) that devices using UWB technology are being developed with transmissi

3、ons that span numerous radiocommunication service allocations; c) that UWB technology may be integrated into many wireless applications such as short-range indoor and outdoor communications, radar imaging, medical imaging, asset tracking, surveillance, vehicular radar and intelligent transportation;

4、 d) that a UWB transmission may be a sequence of short-duration pulses; e) that UWB transmissions may appear as noise-like, which may add to the difficulty of their measurement; f) that the measurements of UWB transmissions are different from those of conventional radiocommunication systems; g) that

5、 proper measurements and assessments of power spectral density are key issues to be addressed for any radiation, noting a) that terms and definitions for UWB technology and devices are given in Recommendation ITU-R SM.1755; b) that there are two general measurement approaches, time domain and freque

6、ncy domain, with each having a particular set of advantages and disadvantages, recommends 1 that techniques described in Annex 1 to this Recommendation should be considered when measuring UWB transmissions. 2 Rec. ITU-R SM.1754 Annex 1 Measurement techniques of ultra-wideband transmissions 1 Introdu

7、ction There are multiple techniques for generating UWB signals with various data modulation and randomization schemes. This Annex describes frequency-domain and time-domain measurement techniques of power spectral density for UWB transmissions and for all types of UWB signals. In this Annex, the ter

8、m “emission” is used in a general sense in the context of measurement, and not with the meaning defined in Article 1 of the Radio Regulations. 1.1 Frequency-domain versus time-domain measurement approaches There are two general approaches for measuring the spectral characteristics associated with UW

9、B emissions, each involving a particular set of advantages and disadvantages. One approach involves the measurement of a UWB signals temporal (time domain) characteristics. Digital signal processing (e.g. Fast Fourier Transform (FFT) is then applied to transform the measured temporal parameters to t

10、heir frequency domain representation. Once the UWB signal has been properly represented in the frequency domain, compliance with bandwidth requirements, emission limits, and other applicable regulations can be determined. The temporal measurement approach is often referred to as a “full-bandwidth” m

11、easurement, since theoretically it yields a characterization of the UWB signal across the full bandwidth. The second approach involves a direct measurement of the UWB spectral characteristics in the frequency domain. This approach, called “swept spectral measurement”, is often referred to as a “band

12、width-limited” measurement, since the bandwidth capabilities of most existing test equipment are considerably less than the full bandwidth of the UWB signal. The temporal measurement approach requires a modern digital storage oscilloscope containing a high-speed digitizer with a real-time bandwidth

13、greater than the upper UWB frequency, and FFT processing to calculate the frequency spectrum of the signal. Post-processing software can include many standard radio-frequency (RF) measurements such as root-mean-square (rms) average power. The swept spectral measurement approach involves the use of a

14、 spectrum analyser, vector signal analyser, or similar measurement instrument to detect the UWB signal characteristics in the frequency domain. Conventional test equipment may be insufficiently sensitive to enable detection of UWB signals at very low levels in specific frequency bands. 1.2 Normal te

15、st signals for data This applies to the equipment under test (EUT) with an external modulation connector. The test data that should be used as an input into EUT for measurement of UWB transmissions should be similar to the data transmitted in the actual operation. In the case of measurements for UWB

16、 communication devices, actual data patterns for the fixed part of control signals and frame structures should be used. However, pseudo-random data patterns may be used for the message part of the signal because the message part may be assumed to be a bit stream that is a random sequence. Rec. ITU-R

17、 SM.1754 3 1.3 General UWB measurement system The measurement of radiated electromagnetic emissions requires the use of a measurement system that comprises a receiving antenna and a test receiver (e.g. a spectrum analyser). When low power signals are involved, a low-noise amplifier (LNA) with a suff

18、icient bandwidth may be needed between the antenna and the test receiver, improving the effective sensitivity of the measurement system. 1.4 Measurement environment The low transmission levels from UWB devices make it desirable to perform the measurement in an anechoic or a semi-anechoic chamber. Me

19、asurements made in an anechoic chamber should correlate to a measurement made in a semi-anechoic chamber. This is usually accomplished by adjusting for the effect of the ground screen in a semi-anechoic environment or an open area test site (OATS). The measure of a devices effective isotropic radiat

20、ed power (e.i.r.p.) should be independent of which type of test environment is used. For frequencies above 1 000 MHz, there is no need for a propagation correction factor since ground reflection is not significant. 1.4.1 Radiated measurement procedure below 1 000 MHz1When the reflection from the gro

21、und screen cannot be eliminated, the following procedure can be used: The UWB emission is examined in small segments, such that reflections, gains and losses do not vary significantly over the segment. For table-top sized devices, place the unit on a non-conducting surface at a height of 0.8 m. Use

22、conventional device rotation and elevation searches to maximize reception of the emission. Take a measurement. Factor in gains and losses, as well as considering the ground screen contribution. Take sufficient measurements both in azimuth and elevation to ascertain that the maximum emission value ha

23、s been recorded. Repeat at each frequency of interest. 1.4.2 Radiated measurement procedure above 1 000 MHz Above 1 000 MHz, in a semi-anechoic chamber, the floor between the device and the receiving antenna is treated with RF absorber to remove the ground screen influence. A scan of the search ante

24、nna over 1 to 4 m should show a maximum emission near the height at which the device has been positioned, if the floor has been properly treated. Note that for a free-space measurement there is no requirement to maintain a device height of 0.8 m. The device may be positioned at any height that maxim

25、ally mitigates reflections from the floor. A highly directive receiving antenna assists in reducing the effect of the ground screen reflection. The measurement is recorded without correction for the ground reflection. 1One administration recognizes 960 MHz as the measurement detector breakpoint in o

26、rder to maintain consistency with its emissions mask which defines an emissions limit breakpoint to coincide with the edge of a worldwide aeronautical radionavigation band. 4 Rec. ITU-R SM.1754 For table-top sized devices, the following procedure can be used: Place the unit on a non-conducting surfa

27、ce at an appropriate height. The floor between the search antenna and the device should be treated with material to absorb RF energy suitable for the frequency range being measured. Vary the height of the search antenna to verify that reflections from the floor have been minimized. It may be necessa

28、ry to alter the height of the device to achieve the lowest reflections from the floor. The main lobe of the search antenna should not receive a floor reflection. The search antenna height should remain fixed throughout the measurement. Take a measurement. Factor in the gains and losses. The ground s

29、creen contribution has been eliminated by the addition of absorber in the reflected path. Take sufficient measurements both in azimuth and elevation to ensure that the maximum value has been recorded. g) Repeat for each frequency of interest. 1.5 Measurement variations for ground penetrating radar d

30、evices and wall imaging radar devices The emissions of concern from ground penetrating radar (GPR) and wall imaging radar (WIR) devices are not those radiated directly from the antenna. Since the direct emissions penetrate a substrate where they are rapidly attenuated, they pose little risk of inter

31、ference to radiocommunication services. Instead, only the indirect (i.e. scattered and/or leaked) emissions are of concern. In order to measure these emissions, a method should be used to isolate the direct emissions from the indirect emissions. Two methods to accomplish this isolation are described

32、 below. One method is to place the GPR/WIR directly over a bed of sand of at least 50 cm in depth. The area of the sand-bed should be adequate to accommodate the GPR/WIR transducer (antenna). Measurements are then performed at an adequate number of radials and antenna height steps to determine the m

33、aximum radiated emission level. If this methodology precludes the use of a ground screen, the measured data should be further adjusted to account for the ground screen contribution. Another method is to place the GPR device at a height of 80 cm on a non-conducting support with the emitter directed d

34、ownwards. If the GPR emissions are expected to have components below 500 MHz, a layer of ferrite tile should be placed directly on the floor below the GPR. Pyramidal or wedge-shaped RF absorbers not less than 60 cm in height are placed directly below the GPR. Some sections of absorber may be inverte

35、d and placed over other absorbers to form a solid block. Care should be taken not to place any RF absorber between the device and the search antenna, as this would prevent energy not directed downwards from reflecting from the ground screen. The placement of the absorber should not be disturbed when

36、 the device is rotated. This arrangement prevents energy directed downward from consideration in the measurement. A search in azimuth and elevation for indirect emissions may now be performed. 1.6 Equipment under test orientation The UWB EUT should be oriented with respect to the measurement system

37、so as to ensure the reception of the maximum radiated signal. Determining this orientation can be made easier by using a non-conductive turntable or other form of positioning system to systematically search for the orientation that provides the maximum response within the measurement system. Regardl

38、ess of how Rec. ITU-R SM.1754 5 the orientation is determined, a sufficient number of radials should be considered to determine the radial at which the maximum response is captured by the measurement system. 1.7 Measurement distance A separation distance of 3 m is normally used. In some cases, it ma

39、y not be possible to measure UWB transmissions without amplification and/or moving to one metre or less separation between the receiving antenna and the UWB device, taking care to maintain the far field condition. 1.8 Measurement antennas Measurement antennas are typically optimized over specific fr

40、equency ranges. When measuring the complete spectrum of UWB transmissions, several measurement antennas are required, each optimized over a distinct frequency range. 1.9 Measurement receiver and detectors The measurement apparatus may be one of the following: a spectrum analyser, an electromagnetic

41、interference (EMI) test receiver, a vector signal analyser, or an oscilloscope. In the following sections, these alternatives are described generically as a measurement receiver. A UWB transmission can exhibit different characteristics depending upon the reference receiver bandwidth. For example, a

42、pulse-generated UWB transmission can appear as a CW-line spectrum if the receiver bandwidth is greater than the pulse repetition frequency (PRF). If the receiver bandwidth is less than the PRF then the same transmission can appear noise-like. In addition, if baseband modulation techniques are used (

43、e.g. pulse position modulation), the spectral lines may be “smeared” within the reference bandwidth, creating a noise-like response. In the case of a line spectrum, the quasi-peak power or peak power spectral density is of particular interest. A noise-like spectrum is best defined in terms of the av

44、erage power spectral density. Due to possible receiver bandwidth dependent variations, the measurement of a UWB spectrum requires the use of several signal detectors. Three signal detectors are recommended for measuring UWB transmissions. For measuring signal characteristics in the radio-frequency s

45、pectrum below 1 000 MHz, a quasi-peak detector specified in CISPR-16-1-1 is recommended. An r.m.s. average detector is recommended for measuring the r.m.s. average UWB radiated signal amplitude in the frequency spectrum above 1 000 MHz. A peak detector is recommended for determining the peak power a

46、ssociated with UWB transmissions in the spectrum above 1 000 MHz. 1.10 Measurement system sensitivity The radiated emissions from a UWB device are often too weak to overcome the noise of a conventional spectrum analyser. For example, noise level of spectrum analyser is equivalent to an e.i.r.p. dens

47、ity of 47 dBm/MHz at one GHz, and 25 dBm/MHz at 26 GHz. Therefore, it becomes necessary to utilize an LNA at the output of the measurement antenna to reduce the effective noise figure of the overall measurement system. This increased sensitivity of the measurement system can render it particularly v

48、ulnerable to ambient environmental signals. If strong ambient signals are present within the measurement environment, an appropriate RF filter should be placed ahead of the LNA to provide the pre-selection necessary to prevent amplifier overload, while permitting signals in the frequency range of in

49、terest to propagate through the measurement system. The insertion loss associated with this filter should be minimal and should also be considered when determining the overall sensitivity of the measurement system. 6 Rec. ITU-R SM.1754 When the analyser sensitivity is insufficient, radiometric measurements described in 2.6 is one of the effective methods. 1.11 Example test sequence The spectral characterization of a UWB device should begin with a peak-detected radiated measurement in a one MHz resolution bandwidth (RBW) since the results obtained from this meas