khonghthesis

Upload: alikurt

Post on 07-Apr-2018

214 views

Category:

Documents


0 download

TRANSCRIPT

  • 8/6/2019 KhongHThesis

    1/61

    FLORIDA STATE UNIVERSITY

    FAMU FSU COLLEGE OF ENGINEERING

    A COMPUTER SIMULATION MODEL FOR MICROWAVE LINK

    PATH LOSS PREDICTION

    By

    HUNG HUY KHONG

    A Thesis submitted to the

    Department of Electrical and Computer Engineeringin partial fulfillment of the

    requirements for the degree ofMaster of Science

    Degree Awarded:

    Summer Semester, 2009

    Copyright 2009

    Hung Huy KhongAll Rights Reserve

  • 8/6/2019 KhongHThesis

    2/61

    ii

    The members of the Committee approve the Thesis of Hung Huy Khong defended on

    April 27th, 2009

    __________________________________________

    Bing W. KwanProfessor Directing Thesis

    _________________________________________

    Leonard J. Tung

    Committee Member

    __________________________________________Simon Y. Foo

    Committee Member

    Approved:

    Victor DeBrunner, Chair, Department of Electrical and Computer Engineering

    Ching-Jen Cheng, Dean, FAMU-FSU College of Engineering

    The Graduate School has verified and approved the above named committee members.

  • 8/6/2019 KhongHThesis

    3/61

  • 8/6/2019 KhongHThesis

    4/61

    iv

    TABLE OF CONTENTS

    LIST OF TABLES .............................................................................................. vi

    LIST OF FIGURES ............................................................................................. vii

    LIST OF ABBREVIATIONS.............................................................................. ix

    ABSTRACT ...................................................................................................... x

    1. INTRODUCTION .......................................................................................... 1

    1.1. Overview of Radio Wave Propagation ................................................ 1

    1.2. Brief Review of Path-loss models........................................................ 3

    1.3. Problem Statement ............................................................................... 5

    1.4. Thesis Organization ............................................................................. 6

    2. NARROWBAND PATH-LOSS MODELS ................................................... 7

    2.1. Free Space Path-loss for LOS Environment ........................................ 7

    2.2. Path-loss for NLOS Environment........................................................ 7

    2.3. Semi-empirical Path-loss Models for Macro-cell Areas...................... 8

    2.3.1. Okumura Model.......................................................................... 9

    2.3.2. Hata Model.................................................................................. 9

    2.3.3. COST-231 Model........................................................................ 11

    2.3.4. Lee Model ................................................................................... 12

    2.3.5. The Model in [3] ......................................................................... 13

    2.3.6. Comparison of Semi-empirical Models...................................... 14

    3. COMPUTER SIMULATION PATH-LOSS MODEL................................... 16

    3.1. Ray Tracing Technique........................................................................ 16

    3.1.1. Two-Ray Model.......................................................................... 16

    3.2. Development of the Computer Simulation Path-loss model................ 18

    3.3. Channel Space...................................................................................... 21

    4. COMPUTER SIMULATION RESULTS....................................................... 23

    4.1. Simulation Procedure........................................................................... 23

    4.2. Statically Regularity of Received Signals............................................ 23

  • 8/6/2019 KhongHThesis

    5/61

  • 8/6/2019 KhongHThesis

    6/61

    vi

    LIST OF TABLES

    Table 2.1: Urban environment correction factors for the Hata model................. 11

    Table 2.2: Suburban and Rural environment correction factors for theHata model......................................................................................... 11

    Table 2.3: Environment parameters for the Lee model ....................................... 13

    Table 2.4: Environment parameters for the model in [3]..................................... 14

    Table 4.1: Mean path loss exponents and intercept values for three differentgroups of objects................................................................................ 33

    Table 4.2: Mean path loss exponents and intercept values for three differentground reflection coefficients ............................................................ 36

  • 8/6/2019 KhongHThesis

    7/61

    vii

    LIST OF FIGURES

    Figure 1.1: A communication system ................................................................. 1

    Figure 2.1: Median loss relative to free space ),( dfAmu .................................. 10

    Figure 2.2: Correction factor AREAG for different environments ..................... 10

    Figure 2.3: Path-loss predicted by Hata, Lee, and the model in [3] for urban area 15

    Figure 3.1: Two-ray model ................................................................................. 17

    Figure 3.2: Two two-ray models characterizing a two-hop multipath signal ..... 19

    Figure 3.3: Channel Space .................................................................................. 21

    Figure 4.1: Typical multipath electric-field phasors received at short distance

    (d= 1 km) withN= 100 scattering objects ....................................... 24

    Figure 4.2: Typical multipath electric-field phasors received at long distance

    (d= 20 km) withN= 100 scattering objects ..................................... 24

    Figure 4.3: Path losses due to 1000 random distributions ofN= 10 scatteringobjects ............................................................................................... 25

    Figure 4.4: The MSE curve fitted through the mean path losses versus logdistance forN= 10 objects yielding a path-loss exponent 0.8

    and intercept 84 dB ........................................................................... 26

    Figure 4.5: Histograms of path loss exponents and intercept values forN= 10

    scattering objects ............................................................................... 27

    Figure 4.6: Histograms of path loss exponents and intercept values forN= 50scattering objects ............................................................................... 27

    Figure 4.7: Histograms of path loss exponents and intercept values forN= 150scattering objects ............................................................................... 28

    Figure 4.8: Path loss based on computer simulations forN= 5 objects.= 0.08and exponent = 0.677 ...................................................................... 30

    Figure 4.9: Path loss based on computer simulations forN= 5 objects.= 0.8and exponent = 2.606 (different object distribution from Figure 4.8) 30

  • 8/6/2019 KhongHThesis

    8/61

  • 8/6/2019 KhongHThesis

    9/61

  • 8/6/2019 KhongHThesis

    10/61

  • 8/6/2019 KhongHThesis

    11/61

    1

    CHAPTER 1

    INTRODUCTION

    1.1. Overview of Radio Wave Propagation

    Figure 1.1: A communication system [17]

    A typical communication system consists of three main systems: the transmitter (TX), the

    receiver (RX) and the transmission channel as depicted in Figure 1.1.

    It is desirable to understand the channels statistical characteristics in order to predict the channel

    behavior. The signal processing techniques then will be developed and used properly to ensure

    that the transmission channel between the TX and the RX is as reliable as possible. Therefore,

    understanding the channel characteristics plays an important role in designing and optimizing a

    communication system.

    The channel is subject to noise, distortion and other interference sources leading to the variation

    of the received signal power. The models that characterize the signal fluctuations over small

    distances in the order of the wavelength or short-time duration are called small-scale models.

    While the propagation models that predict the mean signal strength over the large distances

    between the TX and the RX or long-time duration are called large-scale or path-loss models.

    Destination

    Input

    Signal

    Received

    Signal

    Source

    Transmitted

    Signal Output

    Signal

    Noise, Interference,

    Distortion

    Transmitter ReceiverTransmission

    Channel

  • 8/6/2019 KhongHThesis

    12/61

  • 8/6/2019 KhongHThesis

    13/61

  • 8/6/2019 KhongHThesis

    14/61

    4

    km to 20 km has been proposed by Hata [1], Lee [2], and several other research groups [3, 4].

    Hata proposed the path-loss models for different environments such as urban areas, suburban

    areas, and rural areas based on measurement data. All of these models are similar with respect to

    the signal attenuation rate (path loss exponents). Lee also performed measurement works in

    different cities around the world and proposed alternate path-loss models. Several other research

    groups also investigated the path-loss models for narrowband communication systems based on

    measurement [3]. Those models are applicable not only for different environments, but also for

    varying carrier frequency, antenna heights, the TX-RX separation, etc. For small distances

    between the TX and the RX, several other research groups have also proposed the path-loss

    models for micro-cell areas [4]. It is noticed that all the semi-empirical models predict the

    median path losses.

    There are some techniques used to develop the path-loss model using computer simulation.The

    two-ray models are most commonly used to predict the path loss and calculate the signal

    strength. These models use the ray-tracing technique that is based on geometrical optics to

    account for the three mechanisms discussed above [5, 6]. This technique assumes a finite number

    of multipath signals from the TX to the RX. The knowledge about the physical elements of the

    channel is essential, including the geometry of the scattering objects in the channel. To simplify

    the solution and procedure, however, the ray tracing technique often makes approximations to

    obtain an excess path length. Typically, it is assumed that the nearest scattering objects are in the

    far-field regions of the TX and the RX. In addition, the scattering objects are electrically large [7

    10]. Several research efforts reported in [11 14] have employed the ray-tracing technique. In

    [13], it shows a simple deterministic-plus-stochastic path-loss model for small outdoor areas

    (such as parking lots and intersections). It is found that for these areas with well defined

    geometries, a model (such as 2-ray, 4-ray or multipath reflection model) may be postulated

    initially and the corresponding measurement will be performed to verify the accuracy of the

    assumed models. Simulation results of path loss and delay spread are also presented in [14]. This

    research effort finds that the propagation loss depends on shaped objects and is affected by the

    physical elements of the media, such as the dielectric constants and the roughness factors of the

    objects.

  • 8/6/2019 KhongHThesis

    15/61

    5

    1.3. Problem Statement

    One may notice that the research works described in section 1.2 have several limitations as

    described in the following:

    The collecting measurement data are generally very tedious and costly because largevolume of data needs to be acquired and specialized expensive equipments are involved.

    The measurement data are inherently site-specific and vary from site to site. The ray tracing technique often makes approximations to obtain excess path lengths. Some existing models have been proposed and verified by measurement for very small

    outdoor areas characterized by the TX-RX separation less than 50 meters.

    In view of the limitations described above, it is desirable to have a computer simulation model to

    predict the path loss for different environments and to validate the existing semi-empirical

    models. To achieve this objective, a computer simulation model is proposed that will require

    minimal information about the environment. More specifically, only the number of scattering

    objects and their locations are used to predict the path loss. Such an approach essentially makes

    the proposed model widely applicable to different environments. The added benefit is that it does

    not require the high costs associated with the measurement efforts. Moreover, the computer

    simulation model may lead to criteria for identifying the proper conditions that are best suited for

    a specific existing semi-empirical model.

    To develop a flexible computer model that possesses the attractive features described previously,the following solution approach is taken. Multipath signals resulted from the scattering by any

    number of randomly located objects are considered. Each multipath signal is a two-hop signal

    that involves a single scattering object. The wave (signal) interactions between the TX and a

    scattering object are based on the two-ray model without making restrictive assumptions. The

    same approach is used to account for the wave interactions between a scattering object and the

    RX. The two-ray model considers the effects of wave propagation along the direct path as well

    as the indirect path due to ground reflection. The phase and magnitude of the received signals are

    taken into account in order to properly understand the received signal characteristics. In addition,

    the proposed model allows the flexibility in studying the dependence of path loss on the density

    of scattering objects and the distance between the TX and the RX.

    The key step in the development of the model is the proper representation of the electric field

    due to the direct path and ground-reflected path. The power transmitted from the TX to the

  • 8/6/2019 KhongHThesis

    16/61

  • 8/6/2019 KhongHThesis

    17/61

    7

    CHAPTER 2

    NARROWBAND PATH-LOSS MODELS

    2.1 Free Space Path-loss for LOS Environment

    Free space path loss provides a means to predict the received signal power when there is no

    object obstructing the LOS path between the TX and the RX.

    The model for path loss in a LOS environment is straightforward. The received power rP is

    related to the transmitted power tP via the Friis transmission formula [15]:

    2

    2

    2 )4(4 d

    GGPA

    d

    EIRPP rtter

    ==(W) (2.1)

    In (2.1), ttGPEIRP = . The transmitting antenna has gain tG while the receiving antenna has

    gain rG . Distance d is the separation between the TX and the RX. The RX has an effective

    aperture given by 4/2re GA = , where is the signal wavelength. The path loss is defined by

    the term

    2

    2 44

    ===

    ddG

    A

    GGP

    PL

    r

    e

    rtt

    r

    (2.2)

    It is shown that for the LOS environment, the power received will fall off with the square of the

    distance between the TX and the RX.

    2.2. Path-loss for NLOS Environment

    Since there are scattering objects in the channel, it is quite likely that the transmitted signal

    cannot reach the RX directly since the LOS path is blocked by these objects. These objects can

    greatly impact the average signal strength at the RX.

    Unlike the LOS case, the modeling of path loss in the NLOS environment is more complex and

    involves more environmental parameters in the model. A popular NLOS path-loss model is semi-

    empirical and assumes the form [10], [15]:

  • 8/6/2019 KhongHThesis

    18/61

    8

    [dB])(log10)()(0

    100 dSd

    dndPdL L +

    += (2.3)

    In (2.3), )( 0dPL is the path loss at a reference distance 0d from the TX, S(d) accounts for the

    lognormal shadow fading effects, and n is the path-loss exponent.Many experiments and results have been reported for both LOS and NLOS environments,

    covering the frequency range from 100 MHz to 2 GHz, which is the frequency band for most

    narrowband transmission systems. According to (2.3), path-loss is assumed to be the linear

    function of log distance (to the base 10) with loss exponent n and intercept )( 0dPL . These loss

    exponents and intercept values are subject to change for different environments and generally do

    not equal to the values for LOS environment. Normally the loss exponents and intercept values

    are typically determined by taking several measurements at various distances and performing a

    linear regression to obtain a least square fit to the measured data.

    2.3. Semi-empirical Path-loss Models for Macro-cell Areas

    There are numerous semi-empirical models in the literature aiming to predict the path loss over

    different environments. The models demonstrated below are models derived from measured data

    corresponding to macro cellular environments with path distances ranging from 1 km to over 10

    km. The Hata and Lee models are the most commonly used models for signal prediction in urban

    areas nowadays although they were developed long ago. Many telecommunication providers are

    using these models in designing and optimizing their radio networks. The model in [3] was

    recently developed and will also be compared to the computer simulation model proposed in this

    thesis. The common characteristic of all the models is the linear dependence of path-loss on the

    distance from the TX to the RX, as depicted in (2.3). Various path loss exponents and intercept

    values are reported in these models with respect to different environments. Three typical models:

    the Hata model, the Lee model, and the model in [3], which are best suitable for urban areas, willbe served as the reference for comparison with the proposed computer simulation model reported

    later in Chapter 4.

  • 8/6/2019 KhongHThesis

    19/61

    9

    2.3.1. Okumura Model

    The Okumura model [4] is applied when frequencies range from 150 KHz to 1920 MHz and

    distances from the TX to the RX, range from 1 km up to 100 km. The model is based on

    measured data taken in Japan. This is among the simplest models and becomes the standard for

    path-loss modeling. The standard deviation in predicting the path loss is around 10 dB.

    The model is described by

    AREArtmuF GhGhGdfALdBL += )()(),()( (2.4)

    where L(dB) is the median path loss, FL is the free space path loss calculated by (2.2),

    ),( dfAmu , the median loss relative to free space, is a set of curves developed from measured

    data using omni-directional antennas, )( thG is the base station (BS) gain factor with height th ,

    )( rhG is the MS gain factor with height rh , and AREAG is the environment gain factor. These

    gain factors are given by

    mhmh

    hG tt

    t 301000,200

    log20)( 10 >>

    = (2.5)

    >>

    =

    mhmh

    mhh

    hG

    rr

    rr

    r

    310,3

    log20

    3,3

    log10

    )(

    10

    10

    (2.6)

    The median loss ),( dfAmu and the environment gain factor AREAG are available as Okumura

    curves shown in Figures 2.1 and 2.2.

    2.3.2. Hata Model

    Hata further developed the Okumura model from the semi-empirical path loss data provided by

    Okumura. The Hata model [1] is mostly applicable for urban areas that have not been addressed

    in the Okumura model. The model is best accurate within a frequency range from 150 KHz to

    1500 MHz. The basic formula for the median path lossL(dB) given by Hata is

    KdhhahfdBL kmtrtMHz ++= log)log55.69.44()(log82.13log16.2655.69)( (2.7)

    Where ht and hr are base station and mobile station antenna heights in meters, respectively, dkm

    is the link distance or cell radius in kilometers,fMHz is the centre frequency in megahertz, and the

  • 8/6/2019 KhongHThesis

    20/61

    10

    terms a(hr)and Kare vehicular station antenna height-gain correction factor and environment

    correction factor, respectively, which depend upon the environment. These correction factors for

    different environments are tabulated in Tables 2.1 and 2.2 below.

    Figure 2.1: Median loss relative to free space ),( dfAmu [15]

    Figure 2.2: Correction factor AREAG for different environments [15]

  • 8/6/2019 KhongHThesis

    21/61

    11

    Table 2.1: Urban environment correction factors for the Hata model

    Environment Type K a(hr)

    Urban indoor large city 0MHzfh MHzr 200,0.151.1)54.1log(29.8

    2

    Urban large city 0MHzfh MHzr 200,1.1)54.1log(29.8

    2

    Urban small city 0 )8.0log56.1()7.0log11.1( MHzrMHz fhf

    Table 2.2: Suburban and Rural environment correction factors for the Hata model

    Environment Type K A(hr)

    Suburban 4.528

    log2

    2

    +

    MHzf 0

    Rural indoor (quasi-open) 1094.35log331.18)(log78.4 2 + MHzMHz ff 0

    Rural (quasi-open) countryside

    94.35log331.18)(log78.4 2 + MHzMHz ff 0

    Rural (open) desert 94.40log331.18)(log78.4 2 + MHzMHz ff 0

    2.3.3. COST-231 Model

    COST-231 model [15] is the extended version of the Hata model developed by EURO-COST.

    This model extends the Hata models frequency range from 150 KHz to2000 MHz.The model has a slight difference in the intercept value but the same exponent compared with the

    Hata model. The models path loss is given by

    MkmtrtMHz CdhhahfdBL +++= log)log55.69.44()(log82.13log9.333.46)( (2.8)

  • 8/6/2019 KhongHThesis

    22/61

  • 8/6/2019 KhongHThesis

    23/61

    13

    =

    (W)10

    (W)PowerTransmit3 (2.13)

    =

    4

    dipolehwavelengthalfrespect togain withantennaBS4 (2.14)

    MSatfactorcorrectiongainantennadifferent5 =

    The variable v in 2 equals 2 when the MS antenna height is greater than 10 m and equals 1

    when MS antenna height is smaller than 3 m.

    For convenience, the path-loss models for different environments proposed by Lee are

    summarized as follows:

    [dB]log10)(log)( 01010

    ++=

    of

    fndYXdBL (2.15)

    Table 2.3: Environment parameters for Lee model

    Type of Environment X Y

    Free space 96.92 20

    Open area 86.12 43.5

    US suburban 99.86 38.4

    US urban 108.49 36.8

    Newark, NJ 101.2 43.11

    Tokyo, Japan 123.77 30.5

    2.3.5. The Model in [3]

    The model developed in [3] is best suitable for systems with a carrier frequency of 1.9 GHz and

    base station antenna height of 10 m to 80 m; however, it can be applied to other frequencies with

    a small error. The model is divided into three types according to the environment, namely A, B

    and C. Type A is associated with the maximum path loss and is appropriate for hilly

    environments with moderate to heavy foliage densities. Type C is associated with the minimum

    path loss and applies to flat environments with light tree densities. Type B is characterized with

  • 8/6/2019 KhongHThesis

    24/61

    14

    either mostly flat environments with moderate to heavy tree densities or hilly environments with

    light tree densities. The model may be described as follows:

    00

    10 ,log10)( ddsXXd

    dndBL hf >+++

    += (2.16)

    In (2.16), is the free space path loss given by (2.2), fX is the correction factor for the carrier

    frequency, hX is the correction factor for the mobile station antenna height, s is the shadow

    fading component, which is a zero-mean Gaussian variable, the

    parameter nt

    t xh

    cbhan ++= )( is called the path loss exponent and depends on the base

    station antenna height th and environment type, x is a zero-mean Gaussian variable of unit

    standard deviation ]1,0[ . n normally ranges from 2 to 4. The values of a, b, c, x, and n fordifferent environments are tabulated in Table 2.4 below.

    Table 2.4: Environment parameters for the model in [3]

    Model

    parameter

    Environment

    type A

    Environment

    type B

    Environment

    type C

    a 4.6 4.0 3.6

    b 0.0075 0.0065 0.005

    c 12.6 17.1 20

    n 0.57 0.75 0.59

    2.3.6. Comparison of Semi-empirical Models

    For comparison, the path losses for urban areas predicted by the Hata model, Lee model, and the

    model in [3] for different environments are plotted in Figure 2.3. The specific parameter values

    used for this plot are: antenna heights m2m,70 == rt hh , antenna gains 1== rt GG , and a

    carrier frequency of 900 MHz. The Hata model and the model in [3] for environment A are

  • 8/6/2019 KhongHThesis

    25/61

    15

    applied. The Lee models for different cities including Philadelphia, Newark, and Tokyo are also

    plotted.

    One may observe the path-loss exponent predicted by these models varies from 2 to 4 and the

    intercept value ranges from 90 to 120 dB. These values will be used for comparison later with

    the model proposed in this thesis.

    0 0.2 0.4 0.6 0.8 1 1.2 1.490

    100

    110

    120

    130

    140

    150

    160

    170

    Distance log10(d)

    Pathloss(dB

    )

    Free Space

    Hata Urban

    Lee Philadenphia

    Lee Newark

    Lee Tokyo

    Model in [3]

    n = 3.26

    n = 2

    n = 4.31

    n = 4.2n = 3.68

    n = 3.05

    Figure 2.3: Path-loss predicted by Hata model, Lee model, and the model in [3] for urban areas

  • 8/6/2019 KhongHThesis

    26/61

    16

    CHAPTER 3

    COMPUTER SIMULATION PATH-LOSS MODEL

    3.1. Ray Tracing Technique

    3.1.1. Two-Ray Model

    In this section, the two-ray model based on ray tracing technique, which is the most reasonably

    accurate to predict the path loss and calculate the signal strength, will be presented. This model is

    especially suitable for the urban environments and radio systems that use high tower base station.

    Many research efforts have used the ray-tracing technique in predicting the path loss [7]-[10],

    [11]-[14].

    To account for the rich multipath characteristics of the NLOS environment, it is necessary to

    consider numerous scattering objects in the channel, namely the intervening medium between the

    TX and the RX. For the sake of simplicity, it is assumed that the dominant received signal power

    comes primarily from the one-hop direct signal along the LOS path and the two-hop multipath

    signals due to single reflections.

    The basis of the two-ray model is the proper representation of the electric field incident upon a

    scattering object. The signal at the distance dfrom the transmitting antenna can be expressed in

    terms of the electric field strength of the form:

    )(cos),( 0 dc ttd

    EdtE = (3.1)

    In (3.1), 2/0 EIRPE = with 377= for free space, c is the speed of light, and dt is the

    time delay.

    The two-ray model shown in Figure 3.1 is essential to the development of the multipath model

    that includes an arbitrarily number of reflecting objects. According to (3.1), the total electric

    field at the RX at the distance dfrom the TX is calculated as the sum of the electric field due to

    the LOS path and the ground reflected path.

  • 8/6/2019 KhongHThesis

    27/61

    17

    )/''(cos)'',(

    )/'(cos)',(

    ),(),(),(

    0

    0

    cdt

    d

    EdtE

    cdtd

    EdtE

    dtEdtEdtE

    cgg

    cLOS

    gLOSTOTAL

    =

    =

    +=

    (3.2)

    In (3.2), g denotes the reflection coefficient of the ground.

    Figure 3.1: Two-ray model

    The path difference between the LOS path and the ground reflected path can be well

    approximated by

    d

    hhdd rt

    2''' = (3.3)

    In (3.3), ht and hr are the transmitted and received antenna heights, respectively. The

    approximation is valid as long as the sum of the transmitted and received antenna heights is

    small compared to d. This two-ray model is intended to include the significant effect of the

    ground reflection.

    The phase difference is then defined as

    =

    2(3.4)

  • 8/6/2019 KhongHThesis

    28/61

    18

    Consequently, the total electric field at the RX at the distance d from the TX is computed by

    =

    2sin2),( 0

    d

    EdtETOTAL (3.5)

    As long as the distance d satisfies the condition

    rthh

    d

    20

    > , the total electric field can be

    approximated by

    2),(

    d

    kdtETOTAL = (3.6)

    In (3.6), k is a constant related to 0E , the antenna heights, and the signal wavelength. The

    received power for the two-ray model can be computed as the function of ),( dtETOTAL and the

    path loss is then obtained as

    4

    22

    d

    hh

    GGP

    PL rt

    rtt

    r == (3.7)

    It is seen that the path loss for the two-ray model falls off with the fourth power of the distance

    between the TX and the RX. In our proposed model described subsequently, an arbitrary number

    of two ray models will be applied.

    3.2. Development of the Computer Simulation Path-loss Model

    In this study, an arbitrary number of two-ray models will be applied for developing the path-loss

    model without making any restrictive approximation, which is used by the two-ray model for one

    object presented above.

    In the intervening medium between the TX and the RX, it is assumed that there are numerous

    scattering objects to characterize the rich NLOS multipath environment. Each scattering object

    absorbs the direct signal power from the TX along the LOS path coupled with the indirect signal

    power reflected off the ground. Consider scattering object i as shown in Figure 3.2. It is at

    distance )(1 id from the TX along the LOS path and distance )(1 id along the ground-reflected

    path. The total power absorbed is then re-radiated by object i to RX, which is at distance )(2 id

    along the direct path and distance )(2 id along the ground-reflected path. The power absorbed by

    object i depends on its radar cross section, which is taken to be a circular area with radius )(iR .

  • 8/6/2019 KhongHThesis

    29/61

    19

    Figure 3.2: Two two-ray models characterizing a two-hop multipath signal

    The electric field incident upon scattering object i can be expressed in terms of the electric fieldstrength:

    +=

    )('2

    1

    )(2

    101

    11

    )(')(

    1)(

    idjgidje

    ide

    idEiE

    (3.8)

    In (3.8), 2/0 EIRPE = with intrinsic impedance 377= for free space, and g denotes

    the ground reflection coefficient. The time-average incident signal power density at object i is

    calculated as:

    )(W/m)(2

    1 221)( iES iobject

    = (3.9)

    The EIRP of object i (accounting for the total incident signal power absorbed) is then given by:

    2

    )()()()(

    2

    1)()(

    22122

    1)(iRiE

    iRiEiSiEIRP siobject

    === (3.10)

  • 8/6/2019 KhongHThesis

    30/61

    20

    It is noted in (3.10) that )(is is called the radar cross section of object i . Radar cross section of

    a scattering object is defined as the ratio of the power density of the signal scattered in the

    direction of the RX to the power density of the radio signal incident upon the object [15]. The

    radar cross section can be approximated by the objects surface area. Without loss of generality,

    each object i used in this model is assumed to have a circular shape represented by radius )(iR .

    Therefore, the radar cross section or area surface of object i is given by 2)()( iRis = .

    The corresponding power density due to object i at the RX is then given by:

    22

    221

    22

    1)(8

    )()(

    )(4

    )()(

    id

    iRiE

    id

    iEIRPiSRx

    == (LOS path) (3.11)

    22

    221

    222 )('8

    )()(

    )('4

    )()(

    id

    iRiE

    id

    iEIRPiS

    Rx

    == (Ground-reflected path) (3.12)

    The electric field at the RX due to object i can be expressed by

    )('2

    22

    1)(

    2

    22

    1

    )('2

    2

    )(2

    1

    22

    22

    )('2

    )()(

    )(2

    )()()(

    2)(2)()(

    idj

    g

    idj

    r

    idj

    Rxg

    idj

    Rxr

    eid

    iRiEe

    id

    iRiEiE

    eiSeiSiE

    +=

    += (3.13)

    In an NLOS environment consisting ofNscattering objects, the total electric field at the RX is

    given by the sum

    =

    =N

    irtotal iEE

    1

    )( (3.14)

    The time-average incident signal power density at the RX is given by

    )(W/m2

    1 2*totaltotal EES =

    (3.15)

    Accordingly the total average power received by the RX may be viewed as the average power

    intercepted by the receiving antenna with effective aperture eA and is calculated by

    (W)2

    2total

    eer E

    AASP

    == (3.16)

    Finally, the path loss is then obtained as

    rtt

    r

    GGP

    PL = (3.17)

  • 8/6/2019 KhongHThesis

    31/61

  • 8/6/2019 KhongHThesis

    32/61

  • 8/6/2019 KhongHThesis

    33/61

    23

    CHAPTER 4

    COMPUTER SIMULATION RESULTS

    4.1. Simulation Procedure

    In this section, the simulation result for the path loss presented in the model above will be

    shown. For the computer simulation runs, set km20MHZ,900 0 == sfc . For more

    convenience in calculation, EIRP is set at 1 kW since path loss does not depend on the EIRP.

    The antenna heights m2m,70 == rt hh are used to match the parameters used in measurement

    studies mentioned previously. Their antenna gains are 1== rt GG . The radii of the scattering

    objects vary from 1 m to 5 m. The ground reflection coefficient g is set at 1 (assuming perfect

    reflection). In order to reach statistically meaningful conclusions, 1000 simulation runs are

    performed for a given number of scattering objects N. A typical simulation run involves three

    key steps:

    Step 1: Set the separation distance d between the TX and the RX. Select the number of

    reflecting objects N, then randomly generate their locations ),,( iii zyx and radar cross section

    radii )(iR , Ni ,2,1

    = , such that

    )(,)()(,0 0 iRr|z|iRrxiRsy ii

  • 8/6/2019 KhongHThesis

    34/61

    24

    In the case of small separations, there are fewer dominant received signals scattered by the

    nearby objects as shown in Figure 4.1. These dominant signals vary considerably from

    simulation to simulation, thereby resulting in large variance. In the case of large separations as in

    Figure 4.2, most objects behave more or less equally as distant scatters, thus producing stationary

    signals with smaller variance at the RX.

    0.5 0 0.5 1 1.5 20.6

    0.5

    0.4

    0.3

    0.2

    0.1

    0

    0.1

    0.2

    0.3

    0.4

    Real part of the electric field

    Imaginarypartoftheelectricfield

    Figure 4.1: Typical multipath electric-field phasors received at short distance (d= 1 km) withN= 100 scattering objects

    0.025 0.02 0.015 0.01 0.005 0 0.005 0.01 0.0150.025

    0.02

    0.015

    0.01

    0.005

    0

    0.005

    0.01

    0.015

    Real part of the electric field

    Im

    aginarypartoftheelectricfield

    Figure 4.2: Typical multipath electric-field phasors received at long distance (d= 20 km) with

    N= 100 scattering objects

  • 8/6/2019 KhongHThesis

    35/61

    25

    4.3. Path-loss vs. Distance

    In this computer simulation study, the dependence of path loss on the separation distance d

    between the TX and the RX is of interest. The observation that the variance of the total electric

    field at the TX is smaller at large distances than at small distances as reported in the previous

    section is indeed confirmed by the simulation results depicted in Figure 4.3. Shown in Figure 4.3

    are the path losses due to 1000 random distributions of 100 scattering objects against log

    distance. It clearly indicates that the path loss varies more widely at smaller distances than at

    larger distances. This appears to suggest that the sum of multipath signals tends to reach

    statistical regularity with increasing distance d. In measurement studies, there is no information

    regarding this observation.

    After a typical simulation run corresponding to N scattering objects with a given spatial

    distribution, a straight line is constructed to fit the path losses versus log distance according to

    the mean squared errors (MSE) or least-squares criterion. The slope of this best-fit line gives the

    path-loss exponent, whereas its value at log10(1 km) is the intercept.

    3 3.5 4 4.520

    40

    60

    80

    100

    120

    140

    160

    Distance log10(d)

    Pathloss(dB)

    Figure 4.3: Path losses due to 1000 random distributions ofN= 100 scattering objects

  • 8/6/2019 KhongHThesis

    36/61

    26

    3 3.5 4 4.5

    70

    75

    80

    85

    90

    95

    100

    105

    Distance log10(d)

    Pathloss(dB)

    Figure 4.4: The MSE curve fitted through the mean path losses versus log distance for N= 100

    objects yielding a path-loss exponent 1.69 and intercept 75 dB.

    In Figure 4.4, the mean path loss is plotted against log distance for N= 100 scattering objects.

    The mean path loss at a given distance d is obtained by computing the average of 1000 path loss

    values resulted from simulation. In addition, a minimum MSE curve is fitted through the mean

    path-loss values versus log distance to yield a path-loss exponent 1.69 and an intercept 75 dB.Figures 4.5, 4.6, and 4.7 are the histograms of the path loss exponents and intercepts generated

    from 1000 simulation runs corresponding to the number of scattering objects N= 10, 50, and

    150, respectively. It is evident that the path loss exponents cover the range from 2 to 4, while the

    intercept value varies from 80 dB to 120 dB. These values are in very good agreement with those

    predicted by the Hata model, the Lee model, and the model in [3] as shown in Figure 2.3.

    Another observation is the path loss exponents tend to increase while the path loss intercept

    values tend to decrease with the increase of the number of scattering objects.

  • 8/6/2019 KhongHThesis

    37/61

    27

    5 0 50

    10

    20

    30

    40

    50

    60

    70

    Pathloss exponents

    Frequencycounts

    60 80 100 120 1400

    5

    10

    15

    20

    25

    30

    35

    40

    Pathloss intercept values

    Frequencycounts

    Figure 4.5: Histograms of path loss exponents and intercept values forN= 10 scattering objects

    2 0 2 40

    10

    20

    30

    40

    50

    60

    70

    80

    90

    Pathloss exponents

    Frequencycounts

    40 60 80 100 1200

    5

    10

    15

    20

    25

    30

    35

    Pathloss intercept values

    Frequencycounts

    Figure 4.6: Histograms of path loss exponents and intercept values forN= 50 scattering objects

  • 8/6/2019 KhongHThesis

    38/61

    28

    2 0 2 4 60

    10

    20

    30

    40

    50

    60

    Pathloss exponents

    Frequencycounts

    40 60 80 1000

    5

    10

    15

    20

    25

    30

    35

    Pathloss intercept values

    Frequencycounts

    Figure 4.7: Histograms of path loss exponents and intercept values forN= 150 scattering objects

    4.4. Simulations Key Findings

    4.4.1. Negative Path Loss Exponents

    It may occur as surprising that the histograms of the path loss exponent corresponding to N= 10

    and 50 scattering objects exhibit negative values.

    Specifically in the case when the number of objects N= 10, 16% of the exponents falls below 0,

    81% of the exponents falls between 0 & 2, and 3% falls between 2 and 5.

    A negative path loss exponent means the received signal is stronger than the transmitted signal,

    indicating a physically unrealizable phenomenon. An explanation for such a physically

    impossible result is the assumption that the path loss increases linearly with log distance may not

    be always valid. To gain an understanding of such an abnormal result, the linear correlation of

    the path loss and log distance is examined for two specific cases. The sample correlation

    coefficient of the path loss and log distance is computed according to the formula [16]:

  • 8/6/2019 KhongHThesis

    39/61

    29

    = =

    =

    =M

    m

    M

    mmm

    M

    mmm

    LLdd

    LLdd

    1 1

    22

    1

    )()(

    )()(

    (4.2)

    In (4.2), Mis the number of data points resulted from varying the distances ,,,1, Mmdm =

    between the TX and the RX. The path loss associated with md is denoted by mL . Further,

    ==

    ==M

    mm

    M

    mm L

    MLd

    Md

    11

    1,

    1(4.3)

    The sample correlation coefficient close to 0 indicates a very weak linear relationship between

    the path loss and log distance, whereas close to 1 signifies a strong positive linear relationship.

    In this study, the simulations are conducted for M= 20 TXRX separations, and the distance md

    ranges from 1 km to 20 km. Figure 4.8 depicts the results of simulation runs involving N= 5

    scattering objects. This results in a sample correlation coefficient = 0.08. The subsequent

    MSE-fit curve leads to a path loss exponent equal to 0.677. On the contrary, Figure 4.9

    represents the simulation runs involving N= 5 scattering objects with a different distribution of

    locations but instead have a sample correlation coefficient = 0.8. The resulted MSE-fit curve

    has a path loss exponent equal to 2.606. This strongly suggests that, as decreases toward 0,

    the linear model described by (2.3) may not be always applicable. Otherwise, the linear model

    would yield a negative path loss exponent after applying the MSE curve fitting, especially when

    the number of scattering objects is small. Since the semi-empirical models all have positive path

    loss exponents, it is reasonable to suggest that the number of scattering objects is typically quite

    large in a real environment. Hence, the linear model assumption is generally valid.

  • 8/6/2019 KhongHThesis

    40/61

    30

    3 3.5 4 4.580

    90

    100

    110

    120

    130

    140

    Distance log10(d)

    Pathloss(dB)

    Figure 4.8: Path loss based on computer simulations forN= 5 objects.

    = 0.08 and exponent = 0.677.

    3 3.5 4 4.580

    90

    100

    110

    120

    130

    140

    Distance log10(d)

    Pathloss(dB

    )

    Figure 4.9: Path loss based on computer simulations forN= 5 objects.

    = 0.8 and exponent = 2.606 (different object distribution from Figure 4.8)

    4.4.2. Unnatural Path-loss Exponents

    From Figure 4.5, 4.6 and 4.7 one may notice the unusual result that the path-loss exponents are

    less than 2, which is the natural free-space path loss exponent. It is in fact only natural to expect

  • 8/6/2019 KhongHThesis

    41/61

    31

    the path loss exponent is no less than 2. To seek an explanation for such an unnatural

    phenomenon, the computer simulation is adjusted to make the signals scattered from the objects

    arrive at the RX coherently, namely the signals will add in phase. To ensure phase coherence of

    the multipath signals, the location of scattering object i is so chosen that its distance

    parameters )(and)( 22 idid as depicted in Figure 4.10 satisfy the condition in (19) subject to the

    constraint in (20).

    Ypidid += 2

    2])()('[ 22 (4.4)

    1)(4

    )()2()())((cos1

    2

    22

    222