Narrow- and wideband channels

Transcription

1 RADIO SYSTEMS ETIN15 Lecture no: 3 Narrow- and wideband channels Ove Edfors, Department of Electrical and Information technology Ove.Edfors@eit.lth.se 27 March

2 Contents Short review NARROW-BAND CHANNELS Radio signals and complex notation Large-scale fading Small-scale fading Combining large- and smallscale fading Noise- and interference-limited links WIDE-BAND CHANNELS What makes a channel wide-band? Delay (time) dispersion Narrow- versus wide-band channels 2

3 SHORT REVIEW 3

4 Statistical descriptions of the mobile radio channel POWER [dbw] P TX dbw G TX db L db The propagation loss will change due to movements. These changes of the propagation loss will take place in two scales: G RX db P RX dbw Large-scale: shadowing, slow changes over many wavelengths. Small-scale: interference, fast changes on the scale of a wavelength. Now we are going to approach these variations from a statistical point of view. 4

5 What do we know so far about propagation losses? POWER [dbw Two theoretical expressions for the deterministic propagation loss as functions of distance: P TX dbw G TX db L db G RX db P RX dbw There are other models, which we will discuss later. We have discussed shadowing/ diffraction and reflections, but not really made any detailed calculations. 5

6 RADIO SIGNALS AND COMPLEX NOTATION 6

7 Simple model of a radio signal A transmitted radio signal can be written Amplitude Frequency Phase By letting the transmitted information change the amplitude, the frequency, or the phase, we get the tree basic types of digital modulation techniques ASK (Amplitude Shift Keying) FSK (Frequency Shift Keying) PSK (Phase Shift Keying) Constant envelope 7

8 Example: Amplitude, phase and frequency modulation ( ) = ( ) cos 2p + f ( ) ( ) s t A t f t t A( t ) f ( t) c Comment: 4ASK - Amplitude carries information - Phase constant (arbitrary) PSK - Amplitude constant (arbitrary) - Phase carries information 4FSK Amplitude constant (arbitrary) - Phase slope (frequency) carries information 8

9 The IQ modulator I-channel (in-phase) Transmited radio signal f c -90 o Q-channel (quadrature) Take a step into the complex domain: Complex envelope Carrier factor 9

10 Interpreting the complex notation Complex envelope (phasor) Transmitted radio signal Polar coordinates: By manipulating the amplitude A(t) and the phase Φ(t) of the complex envelope (phasor), we can create any type of modulation/radio signal. 10

11 LARGE-SCALE FADING 11

12 A narrowband system described in complex notation (noise free) Transmitter Channel Receiver In: Out: Attenuation Phase It is the behaviour of the channel attenuation and phase we are going to model. 12

13 Large-scale fading Basic principle Received power D C Position d A B Movement A B C C 13

14 Large-scale fading More than one shadowing object Signal path in terrain with several diffraction points adding extra attenuation to the pathloss. This is ONE explanation Total pathloss: Deterministic If these are considered random and independent, we should get a normal distribution in the db domain. 14

15 Large-scale fading Log-normal distribution Measurements confirm that in many situations, the large-scale fading of the received signal strength has a normal distribution in the db domain. POWER [dbw] Note db scale P TX dbw L db Deterministic mean value of path loss, L 0 db db P RX dbw Standard deviation 15

16 Large-scale fading Fading margin We know that the path loss will vary around the deterministic value predicted. We need to design our system with a margin allowing us to handle higher path losses than the deterministic prediction. This margin is called a fading margin. Increasing the fading margin decreases the probability of outage, which is the probability that our system receive a too low power to operate correctly. 16

17 Large-scale fading Fading margin (cont.) Fading margin Designing the system to handle an M db db higher loss than predicted, lowers the probability of outage. L 0 db db The upper tail probability of a unit variance, zero-mean, Gaussian (normal) variable: The complementary error-function can be found in e.g. MATLAB 17

18 The Q(.)-function Upper-tail probabilities x Q(x) x Q(x) x Q(x)

19 Large-scale fading A numeric example How many db fading margin, against σ F db = 7 db log-normal fading, do we need to obtain an outage probability of 0.5%? Consulting the Q(.)-function table (or using a numeric software), we get 19

20 SMALL-SCALE FADING 20

21 Small-scale fading Ilustration shown during Lecture 1 Received power [log scale] Illustration of interference pattern from above A Movement B A Position B Transmitter Reflector Many reflectors... let s look at a simpler case! 21

22 Small-scale fading Two waves Wave 1 Wave 1 + Wave 2 Wave 2 At least in this case, we can see that the interference pattern changes on the wavelength scale. 22

23 Small-scale fading Many incoming waves Many incoming waves with independent amplitudes and phases Add them up as phasors 3 r 3 φ r 2 2 r1 1 r 4 r 4 23

24 Small-scale fading Rayleigh fading No dominant component (no line-of-sight) TX X RX Tap distribution 2D Gaussian (zero mean) Amplitude distribution 0.8 Rayleigh 0.6 Im ( a ) Re( a) r No line-of-sight component 24

25 Small-scale fading Rayleigh fading Fading margin Rayleigh distribution Fading margin r min 0 r r rms = 2s Probability that the amplitude r is below some threshold r min : 25

26 Small-scale fading A numeric example How many db fading margin, against Rayleigh fading, do we need to obtain an outage probability of 1%? Some manipulation gives 26

27 Small-scale fading Doppler shifts Frequency of received signal: Receiving antenna moves with speed s RX at an angle θ relative to the propagation direction of the incoming wave, which has frequency f 0. c where the Doppler shift is The maximal Doppler shift is [c = speed of light = 3x10 8 m/s] 27

28 Small-scale fading Doppler spectrum Incoming waves from several directions (relative to movement or RX) Spectrum of received signal when a f 0 Hz signal is transmitted. RX movement RX 4 3 All waves of equal strength in this example, for simplicity. 28

29 Small-scale fading Doppler spectrum Isotropic uncorrelated scattering RX movement 1 Time correlaion RX Uncorrelated amplitudes and phases Uniform incoming power distribution (isotropic) 29

30 Small-scale fading The Doppler spectrum For the uncorrelated scattering with uniform angular distribution of incoming power (isotropic scattering), we obtain the Doppler spectrum by Fourier transformation of the time correlation of the signal: SD Doppler spectrum at center frequency f 0. ( n - f ) 0 for This is the classical Doppler spectrum, a.k.a. the Jakes doppler spectrum. 30

31 Small-scale fading Fading dips Received amplitude [db] Time The larger the fading margin, the rarer the fading dips, and the shorter they are. The length and the frequency of fading dips can be important for the functionality of a radio system. Can we quantify these? 31

32 Small-scale fading Statistics of fading dips Frequency of the fading dips (normalized dips/second) Length of fading dips (normalized dip-length) These curves are for Rayleigh fading and isotropic uncorrelated scattering (Jakes doppler spectrum). 32

33 Small-scale fading Rice fading Tap distribution 2D Gaussian (non-zero mean) A Im ( a ) Re( a) A dominant component (line of sight) Amplitude distribution Rice k = 30 k = 10 k = 0 TX RX Line-of-sight (LOS) component with amplitude A. Power in LOS component k= Power in random components = A

34 COMBINING LARGE- AND SMALL-SCALE FADING 34

35 Large- and small-scale fading Combining the two We will start using Alternative 1 We have seen examples of how we can compute the required fading margins, due to large- and small-scale fading, given certain criteria (e.g. outage probability). There are basically two options: 1) Calculate the fading margins separately and add them up. 2) Derive the pdf (or cdf) of the total fading and calculate a single fading margin for both. If we have both types of fading, how do we combine them into a total fading margin? Alternative 1 is the simple solution, but it will overdimension the system a bit. Alternative 2 is a much more complex operation. 35

36 NOISE- AND INTERFERENCE- LIMITED LINKS 36

37 Noise-limited system Fading margin and the link budget P TX dbm POWER [dbm] Fading L 0 db C 0 db m M db ( C / N ) min N db m Noise reference level Fading C min db m db We use some propagation model to calculate a deterministic propagation loss. Variations in the environment and movements will cause variations in the the propagation loss, which will influence the instantaneous received power. To protect the receiver from too low received power, we add a fading margin. Requirement for the receiver to operate properly. 37

38 Interference-limited system Interference fadning margin TX-A ( C / I ) min db RX-A Received power [db] C dmax Taking fading into account Without taking fading into account I TX-B ( C I ) + M / min db db Distance In interference limited systems, we are preliminary interested in how far from the transmitter we can be, without receiveing too much interference. Depending on the system design and requirements on quality, our receiver can tolerate a certain (C/I) min. Assuming fading on the wanted and interfering signal we can calculate a fading margin M db required to fulfill som criterion on e.g. outage. For independent log-normal fading, we can add the variances of the two fading characteristics and get a total lognormal fading with standard deviation: 2 2 s = s + s tot db C db I db 38

39 DELAY (TIME) DISPERSION 39

40 Delay (time) dispersion A simple case Transmitted impulse t Received signal (channel impulse response) t 1 a 1 t 2 a 2 a 3 t 3 t 40

41 Delay (time) dispersion One reflection/path, many paths Since each bin consists of contributions from several waves, each bin will fade if we introduce movement. Impulse response Delay in excess of direct path Each bin consists of incoming waves that are too close in time to resolve. What do we mean by too close in time? 41

42 Delay (time) dispersion Bandwidth and time-resolution Radio systems are band-limited, which makes our infinitely short impulses become waveforms with a certain width in time. Band-limiting to B Hz The time-width of the pulses is inversely proportional to the bandwidth. 42

43 NARROW- VERSUS WIDE-BAND 43

44 Narrow- versus wide-band Channel impulse response The same radio propagation environment is experienced differently, depending on the system bandwidth. High BW Medium BW Low BW 44

45 Narrow- versus wide-band Channel frequency response f A narrow-band system (bandwidth B 1 ) will not experience any significant frequency selectivity or delay dispersion. A wide-band system (bandwidth B 2 ) will however experience both frequency selectivity and delay dispersion. Note that narrow- or wide-band depends on the relation between channel properties and system bandwidth. It is not an absolute measure. 45

46 Narrow- versus wide-band Let s not forget the time-dependence! We need to take absolute time t into consideration, as the channel will change when things move. Measurement in hilly terrain at 900 MHz. The channel impulse response becomes: Clock time Delay [Liebenow & Kuhlmann 1993] 46

47 Narrow- versus wide-band Doppler spectrum and delay Since the channel at each delay τ is the result of different propagation paths, we can have different Doppler spectra for each delay. Measurement in hilly terrain at 900 MHz. This effect is shown by the scattering function: (received power as function of doppler shift and delay) 47

48 Summary NARROW-BAND CHANNELS Complex notation with amplitude, phase and complex envelope (phasor). Large-scale fading with log-normal distribution and calculation of fading margin. Small-scale fading with Rayleig and Rice distribution, calculation of fading margin. Received signal maximal Doppler shift, Doppler spectrum and time characteristics. Fading margin in the link-budget of noise limited systems. Fading margin and maximal distance for interference limited systems. WIDE-BAND CHANNELS Instead of one (time varying) channel coefficient, we have an entire (time varying) impulse response Channel delay (time) dispersion and frequency selectivity Doppler spectrum as function of delay, i.e. the scattering function There is MUCH MORE to learn about this which many of you have done in the Channel Modeling course (ETIN10)! 48