Session2 Antennas and Propagation
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1 Wireless Communication Presented by Dr. Mahmoud Daneshvar Session2 Antennas and Propagation 1. Introduction Types of Anttenas Free space Propagation 2. Propagation modes 3. Transmission Problems 4. Fading 1
2 1. Introduction An antenna is an electrical conductor or system of conductors Transmission - radiates electromagnetic energy into space Reception - collects electromagnetic energy from space In two-way communication, the same antenna can be used for transmission and reception 2
3 Radiation Patterns Radiation pattern Graphical representation of radiation properties of an antenna Depicted as two-dimensional cross section Beam width (or half-power beam width) Measure of directivity of antenna Reception pattern Receiving antenna s equivalent to radiation pattern 3
4 Types of Antennas Isotropic antenna (idealized) Radiates power equally in all directions Dipole antennas Half-wave dipole antenna (or Hertz antenna) Quarter-wave vertical antenna (or Marconi antenna) Parabolic Reflective Antenna 4
5 5
6 6
7 7
8 8
9 Antenna Gain Antenna gain Measure of the directionality of an antenna Power output, in a particular direction, compared to that produced in any direction by a perfect omnidirectional antenna (isotropic antenna) Effective area Related to physical size and shape of antenna 9
10 Free-space propagation Transmitted power P T Omni-directional transmitting antenna d Received power P ) R Receiving antenna, area A R where is an efficiency parameter Focusing capability: determined by the antenna size in wavelenths (the wavelength is λ): where is the transmitting antenna efficiency factor 10
11 Directional antenna Transmitted power P ( T d Received power P ) R Transmitting antenna, area A T Receiving antenna, area AR Directional antenna gain G T > 1 Similarly to what done on previous slide: Hence: free-space received power: 11
12 2. Propagation Modes Ground-wave propagation Sky-wave propagation Line-of-sight propagation 12
13 13
14 Ground Wave Propagation 14
15 Ground Wave Propagation Follows contour of the earth The electromagnetic wave induces a current in hte earth s surface the waveform tilts downwards Diffraction Can Propagate considerable distances Frequencies up to 2 MHz Example AM radio 15
16 Sky Wave Propagation 16
17 Sky Wave Propagation Signal reflected from ionized layer of atmosphere back down to earth Signal can travel a number of hops, back and forth between ionosphere and earth s surface Reflection effect caused by refraction Examples Amateur radio CB radio 17
18 Line-of-Sight Propagation 18
19 Line-of-Sight Propagation Required above 30 MHz Transmitting and receiving antennas must be within line of sight Satellite communication signal above 30 MHz not reflected by ionosphere Ground communication antennas within effective line of site due to refraction Refraction bending of microwaves by the atmosphere Velocity of electromagnetic wave is a function of the density of the medium When wave changes medium, speed changes Wave bends at the boundary between mediums 19
20 20
21 Line-of-Sight Equations Optical line of sight d Effective, or radio, line of sight h d h d = distance between antenna and horizon (km) h = antenna height (m) K = adjustment factor to account for refraction, rule of thumb K = 4/3 21
22 Line-of-Sight Equations Maximum distance between two antennas for LOS propagation: 3.57 h h 1 2 h 1 = height of antenna one h 2 = height of antenna two 22
23 3. Transmission problems Attenuation Free space loss attenuation distortion Noise Atmospheric absorption Multipath Refraction 23
24 Attenuation Strength of signal falls off with distance over transmission medium Attenuation factors for unguided media: Received signal must have sufficient strength so that circuitry in the receiver can interpret the signal Signal must maintain a level sufficiently higher than noise to be received without error Attenuation is greater at higher frequencies, causing distortion 24
25 Free Space Loss Free space loss, ideal isotropic antenna P t P r 2 4d 4fd l 2 P t = signal power at transmitting antenna P r = signal power at receiving antenna l = carrier wavelength d = propagation distance between antennas c = speed of light m/s) where d and l are in the same units (e.g., meters) c
26 Free Space Loss Free space loss equation can be recast: L db 10log Pt P r 20log 4d l l 20logd db 20log 4fd 20log 20log c f 20logd db 26
27 27
28 Free Space Loss Free space loss accounting for gain of other kinds of antennas P t P r d ld cd G G r t l 2 A r A t f 2 A r 2 A t G t = gain of transmitting antenna G r = gain of receiving antenna A t = effective area of transmitting antenna A r = effective area of receiving antenna 28
29 Free Space Loss Free space loss accounting for gain of other kinds of antennas can be recast as L db l 20logd 10logA A 20log f 20log d 10log A A t dB 20log t r r 29
30 Categories of Noise Thermal Noise Intermodulation noise Crosstalk Impulse Noise 30
31 Thermal Noise Also called white noise Due to agitation of electrons Present in all electronic devices and transmission media Cannot be eliminated Function of temperature Particularly significant for satellite communication 31
32 Thermal Noise Amount of thermal noise to be found in a bandwidth of 1Hz in any device or conductor is: N kt 0 W/Hz N 0 = noise power density in watts per 1 Hz of bandwidth k = Boltzmann's constant = J/K T = temperature, in kelvins (absolute temperature) 32
33 Thermal Noise Noise is assumed to be independent of frequency Thermal noise present in a bandwidth of B Hertz (in watts): N ktb N or, in decibel-watts 10log k 10 log T 10log B dbw 10 log T 10log B 33
34 Noise Terminology Intermodulation noise occurs if signals with different frequencies share the same medium Interference caused by a signal produced at a frequency that is the sum or difference of original frequencies Crosstalk unwanted coupling between signal paths Impulse noise irregular pulses or noise spikes Short duration and of relatively high amplitude Caused by external electromagnetic disturbances, or faults and flaws in the communications system 34
35 Expression E b /N 0 Ratio of signal energy per bit to noise power density per Hertz E b S / R S N N ktr where S is the signal power, R the bitrate, k Boltzmann s constant and T the temperature The bit error rate for digital data is a function of E b /N Given a value for E b /N 0 to achieve a desired error rate, parameters of this formula can be selected As bit rate R increases, transmitted signal power must increase to maintain required E b /N 0 35
36 36
37 Other Impairments Atmospheric absorption water vapor and oxygen contribute to attenuation Multipath obstacles reflect signals so that multiple copies with varying delays are received Refraction bending of radio waves as they propagate through the atmosphere 37
38 4. Fading Fading: time variation of received signal power due to changes in the transmission medium or path(s) Kinds of fading: Fast fading Slow fading Flat fading independent from frequency Selective fading frequency-dependent Rayleigh fading no dominant path Rician fading Line Of Sight (LOS) is dominating + presence of indirect multipath signals 38
39 39
40 Multipath Propagation Reflection - occurs when signal encounters a surface that is large relative to the wavelength of the signal Diffraction - occurs at the edge of an impenetrable body that is large compared to wavelength of radio wave Scattering occurs when incoming signal hits an object whose size in the order of the wavelength of the signal or less 40
41 Multipath Propagation 41
42 The Effects of Multipath Propagation Multiple copies of a signal may arrive at different phases If phases add destructively, the signal level relative to noise declines, making detection more difficult Intersymbol interference (ISI) One or more delayed copies of a pulse may arrive at the same time as the primary pulse for a subsequent bit 42
43 Propagation Characteristics Path Loss (includes average shadowing) Shadowing (due to obstructions) Multipath Fading P t P r v P r /P t Slow Fast Very slow d=vt d=vt
44 Path Loss Modeling Maxwell s equations Complex and impractical Free space path loss model Too simple Ray tracing models Requires site-specific information Empirical Models Don t always generalize to other environments Simplified power falloff models Main characteristics: good for high-level analysis
45 Free Space (LOS) Model d=vt Path loss for unobstructed LOS path Power falls off : Proportional to d 2 Proportional to l 2 (inversely proportional to f 2 )
46 Ray Tracing Approximation Represent wavefronts as simple particles Geometry determines received signal from each signal component Typically includes reflected rays, can also include scattered and defracted rays. Requires site parameters Geometry Dielectric properties
47 Two Path Model Path loss for one LOS path and 1 ground (or reflected) bounce Ground bounce approximately cancels LOS path above critical distance Power falls off Proportional to d 2 (small d) Proportional to d 4 (d>d c ) Independent of l (f)
48 General Ray Tracing Models all signal components Reflections Scattering Diffraction Requires detailed geometry and dielectric properties of site Similar to Maxwell, but easier math. Computer packages often used
49 Simplified Path Loss Model Used when path loss dominated by reflections. Most important parameter is the path loss exponent g, determined empirically. P r PK t g d 0, 2 g d 8
50 Empirical Models Okumura model Empirically based (site/freq specific) Awkward (uses graphs) Hata model Analytical approximation to Okumura model Cost 136 Model: Extends Hata model to higher frequency (2 GHz) Walfish/Bertoni: Cost 136 extension to include diffraction from rooftops Commonly used in cellular system simulations
51 Main Points Path loss models simplify Maxwell s equations Models vary in complexity and accuracy Power falloff with distance is proportional to d 2 in free space, d 4 in two path model General ray tracing computationally complex Empirical models used in 2G simulations Main characteristics of path loss captured in simple model P r =P t K[d 0 /d] g
52 52
53 53
54 K Power in the dominant path Power in the scattered paths K=0 : Rayleigh K= : Additive White Gaussian Noise 54
55 Solution Error Compensation Mechanisms Adaptive Equalization Diversity Techniques 55
56 Error Compensation Mechanisms Forward error correction Adaptive equalization Diversity techniques 56
57 Forward Error Correction Transmitter adds error-correcting code to data block Code is a function of the data bits Receiver calculates error-correcting code from incoming data bits If calculated code matches incoming code, no error occurred If error-correcting codes don t match, receiver attempts to determine bits in error and correct 57
58 Adaptive Equalization Can be applied to transmissions that carry analog or digital information Analog voice or video Digital data, digitized voice or video Used to combat intersymbol interference Involves gathering dispersed symbol energy back into its original time interval Techniques Lumped analog circuits Sophisticated digital signal processing algorithms 58
59 A known training sequence is sent periodically. The receiver fine tunes the coefficients accordingly. 59
60 Diversity Techniques Diversity is based on the fact that individual channels experience independent fading events Space diversity techniques involving physical transmission path (e.g., multiple antennas) Frequency diversity techniques where the signal is spread out over a larger frequency bandwidth or carried on multiple frequency carriers Time diversity techniques aimed at spreading the data out over time 60
61 61
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