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TURKEY RADAR TRAINING 1.0 / ALANYA 2005<br />

TURKISH STATE METEOROLOGICAL SERVICE<br />

(TSMS)<br />

WORLD METEOROLOGICAL ORGANIZATION<br />

(WMO)<br />

COMMISSION FOR INSTRUMENTS AND METHODS OF OBSERVATIONS<br />

(CIMO)<br />

OPAG ON CAPACITY BUILDING (OPAG-CB)<br />

EXPERT TEAM ON TRAINING ACTIVITIES AND TRAINING MATERIALS<br />

TRAINING COURSE ON<br />

WEATHER RADAR SYSTEMS<br />

MODULE A: INTRODUCTION TO RADAR<br />

ERCAN BÜYÜKBAŞ-Electr<strong>on</strong>ics Engineer<br />

OĞUZHAN ŞİRECİ -Electr<strong>on</strong>ics Engineer<br />

AYTAÇ HAZER -Electr<strong>on</strong>ics Engineer<br />

İSMAİL TEMİR -Mechanical Engineer<br />

ELECTRONIC OBSERVING SYTEMS DIVISION<br />

TURKISH STATE METEOROLOGICAL SERVICE<br />

12–16 SEPTEMBER 2005<br />

WMO RMTC-TURKEY<br />

ALANYA FACILITIES, ANTALYA, TURKEY


INTRODUCTION TO RADAR<br />

CONTENTS<br />

1 INTRODUCTION 2<br />

1.1. A few words <strong>on</strong> that <str<strong>on</strong>g>course</str<strong>on</strong>g> 2<br />

1.2. A few words <strong>on</strong> <strong>weather</strong> <strong>radar</strong>s 3<br />

2 RADAR THEORY 5<br />

2.1.The history of <strong>radar</strong> 5<br />

2.2.Basic Radar Terms 7<br />

2.3.Operati<strong>on</strong> Principle of Radars 9<br />

2.4.Radar Equati<strong>on</strong> 10<br />

2.5.Block Diagram of a Radar 23<br />

3 PROPOGATION OF EM WAVES 26<br />

3.1.Electromagnetic Spectrum 26<br />

3.2. Electromagnetic Waves 28<br />

3.2.1. Polarizati<strong>on</strong> 29<br />

3.3. Refracti<strong>on</strong> 32<br />

3.3.1. Refractive Index 32<br />

3.3.2. Curvature 33<br />

4 RADAR TYPES 34<br />

4.1. M<strong>on</strong>ostatic Radars 35<br />

4.2. Bistatic Radars 35<br />

4.3. Air Surveillance Radars 35<br />

4.4. 3-D Radars 36<br />

4.5. Synthetic Aperture Radars 36<br />

4.6. C<strong>on</strong>tinuous Wave Radars 36<br />

4.7. FM-CW Radars 37<br />

4.8. Moving Target Indicati<strong>on</strong> Radars 37<br />

4.9. Pulse Radars 38<br />

4.10. Doppler Radars 38<br />

4.11. Weather Radars 39<br />

4.12. Polarimetric Radars 40<br />

4.13. Terminal Doppler Weather Radars (TDWR) 41<br />

4.14. Wind Profiler Radars 41<br />

4.15. Mobile Radars 43<br />

5 REFERENCES 44


MODULE A- INTRODUCTION TO RADAR<br />

1. INTRODUCTION<br />

1.1. A few words <strong>on</strong> that <str<strong>on</strong>g>course</str<strong>on</strong>g><br />

Recently, Turkish State Meteorological Service (TSMS) started a modernizati<strong>on</strong> program of<br />

observing <strong>systems</strong> including <strong>weather</strong> <strong>radar</strong>s. So a great knowledge have been transferred to the staff<br />

of TSMS by means of installati<strong>on</strong> high technology <strong>weather</strong> <strong>radar</strong>s, getting <str<strong>on</strong>g>training</str<strong>on</strong>g> <str<strong>on</strong>g>course</str<strong>on</strong>g>s from<br />

<strong>radar</strong> manufacturers and internati<strong>on</strong>al experts both <strong>on</strong> operati<strong>on</strong>/interpretati<strong>on</strong> and<br />

maintenance/calibrati<strong>on</strong> of <strong>weather</strong> <strong>radar</strong>s. As a result of those very important activities, TSMS has<br />

caught e very important level <strong>on</strong> <strong>weather</strong> <strong>radar</strong> applicati<strong>on</strong>s. And then as an active member of<br />

WMO <strong>on</strong> Regi<strong>on</strong>al Metrological <strong>Training</strong> Activities, TSMS has planed to organize regular <str<strong>on</strong>g>training</str<strong>on</strong>g><br />

activities <strong>on</strong> <strong>weather</strong> observing <strong>systems</strong> in line with the tasks of Expert Team <strong>on</strong> <strong>Training</strong> Materials<br />

and <strong>Training</strong> Activities established by CIMO Management Group (OPAG <strong>on</strong> Capacity Building<br />

(OPAG-CB)/C.1. Expert Team <strong>on</strong> <strong>Training</strong> Activities and <strong>Training</strong> Materials).<br />

The <str<strong>on</strong>g>training</str<strong>on</strong>g> <str<strong>on</strong>g>course</str<strong>on</strong>g> organized by Turkish State Meteorological Service <strong>on</strong> <strong>weather</strong> <strong>radar</strong> <strong>systems</strong><br />

and <str<strong>on</strong>g>training</str<strong>on</strong>g> documents prepared for that <str<strong>on</strong>g>training</str<strong>on</strong>g> <str<strong>on</strong>g>course</str<strong>on</strong>g> are intended to give a general informati<strong>on</strong><br />

<strong>on</strong> <strong>radar</strong> theory, <strong>weather</strong> <strong>radar</strong>s and meteorological applicati<strong>on</strong>s, to highlight the important topics, to<br />

summarize the critical aspects by reviewing the informati<strong>on</strong> and comments from different sources<br />

and to provide some vital informati<strong>on</strong> why and how to install and operate a <strong>weather</strong> <strong>radar</strong> network.<br />

All these activities must be understood and accepted as just a key for opening a small door to the<br />

complex and great world of <strong>radar</strong>s, particularly Doppler <strong>weather</strong> <strong>radar</strong>s. Furthermore, we believe<br />

that such organizati<strong>on</strong>s will help the experts from different countries and community of<br />

meteorology will come closer. In additi<strong>on</strong>, exchange of the experiences will support the capacity<br />

building activities extremely.<br />

The <str<strong>on</strong>g>training</str<strong>on</strong>g> documents have been prepared by reviewing the popular <strong>radar</strong> books and the other<br />

documents available. On the other hand, a lot of useful informati<strong>on</strong> has been provided from the<br />

internet. TSMS has got very effective <str<strong>on</strong>g>training</str<strong>on</strong>g> <str<strong>on</strong>g>course</str<strong>on</strong>g> from the <strong>radar</strong> manufacturers who supplied<br />

the existing <strong>radar</strong>s operated by TSMS. <strong>Training</strong> documents prepared during those <str<strong>on</strong>g>course</str<strong>on</strong>g>s and notes<br />

from the lectures are the other important sources of those <str<strong>on</strong>g>training</str<strong>on</strong>g> materials. Radar manufacturers’<br />

dem<strong>on</strong>strati<strong>on</strong>s and power point presentati<strong>on</strong>s by experts have also been taken into c<strong>on</strong>siderati<strong>on</strong><br />

while preparing the documents.<br />

2<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005


MODULE A- INTRODUCTION TO RADAR<br />

<strong>Training</strong> materials have been prepared as a set of 6 (six) separate modules. But modules are directly<br />

related to each other for completi<strong>on</strong> of the topics covered by <str<strong>on</strong>g>training</str<strong>on</strong>g> <str<strong>on</strong>g>course</str<strong>on</strong>g>. Modules supplement<br />

each other.<br />

It is very obvious that, as being our first <str<strong>on</strong>g>training</str<strong>on</strong>g> <str<strong>on</strong>g>course</str<strong>on</strong>g> and first <str<strong>on</strong>g>training</str<strong>on</strong>g> documents regarding<br />

<strong>radar</strong>s in English, those <str<strong>on</strong>g>training</str<strong>on</strong>g> documents, most probably, will be in need of reviewed and<br />

modified in some topics. Whoever makes any comment, recommendati<strong>on</strong>s and correcti<strong>on</strong>s will be<br />

highly appreciated. We think those invaluable c<strong>on</strong>tributi<strong>on</strong>s will pave our way for further activities.<br />

1.2. A few words <strong>on</strong> <strong>weather</strong> <strong>radar</strong>s<br />

To watch the atmosphere and the <strong>weather</strong> phenomena occurred is getting more and more important<br />

for the developing world. To be able to meet the meteorological requirements of the developing<br />

world, it is very obvious that there is a necessity for the provisi<strong>on</strong> of accurate and timely <strong>weather</strong><br />

observati<strong>on</strong>s which will be the essential input of <strong>weather</strong> forecasts and numerical <strong>weather</strong><br />

predicti<strong>on</strong> models, research studies <strong>on</strong> climate and climate change, sustainable development,<br />

envir<strong>on</strong>ment protecti<strong>on</strong>, renewable energy sources, etc. All outputs and products of any system are<br />

input dependant. So, accuracy, reliability and efficiency of the products of any meteorological study<br />

will depend <strong>on</strong> its input: Observati<strong>on</strong>.<br />

It is vital to observe the <strong>weather</strong> and to make <strong>weather</strong> predicti<strong>on</strong> timely especially for severe<br />

<strong>weather</strong> c<strong>on</strong>diti<strong>on</strong>s to be able to warn the public in due <str<strong>on</strong>g>course</str<strong>on</strong>g>. One of the most important and<br />

critical instruments developed and offered by the modern technology for observing <strong>weather</strong> and<br />

early warning <strong>systems</strong> are <strong>weather</strong> <strong>radar</strong>s. It would not be a wr<strong>on</strong>g comment to say that <strong>radar</strong> is the<br />

<strong>on</strong>ly and essential sensor which can provide real time and accurate informati<strong>on</strong> <strong>on</strong> hazardous<br />

<strong>weather</strong> phenomena such as str<strong>on</strong>g wind, heavy precipitati<strong>on</strong> and hail in large scale area.<br />

Doppler and wind profiling <strong>radar</strong>s are proving to be extremely valuable in providing data of highresoluti<strong>on</strong><br />

in both space and, especially in the lower layers of the atmosphere. Doppler <strong>radar</strong>s are<br />

used extensively as part of nati<strong>on</strong>al, and increasingly of regi<strong>on</strong>al networks, mainly for short range<br />

forecasting of severe <strong>weather</strong> phenomena. Particularly useful is the Doppler <strong>radar</strong> capability of<br />

making wind measurements and estimates of rainfall amounts. Wind profiler <strong>radar</strong>s are especially<br />

useful in making observati<strong>on</strong>s between ballo<strong>on</strong>-borne soundings, and have great potential as a part<br />

of integrated observing networks.<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005 3


MODULE A- INTRODUCTION TO RADAR<br />

Hydrologists need precipitati<strong>on</strong> measurements. As simple as it looks, as difficult it is to obtain<br />

reliable data. We know that rain gauge measurements have errors, owing to the type of the<br />

instrument and to the site. Wind, snowfall, drop-size influence the results. But the largest problem is<br />

the areal representativeness. Measurements <strong>on</strong> a surface of 200 or 400 cm2 are used to estimate the<br />

rainfall <strong>on</strong> areas in the order of magnitude of 100 km2. Knowing the spatial variability of rainfall,<br />

especially during flood events, it is obvious that point measurements, even if the measurement itself<br />

would be correct, are heavily biased.<br />

The hope of hydrologists and meteorologists is c<strong>on</strong>centrated <strong>on</strong> <strong>radar</strong> measurements. Radar<br />

provides images of instantaneous rainfall intensity distributi<strong>on</strong> over large areas. However, when<br />

trying to obtain the desired quantitative results <strong>on</strong>e encounters a series of problems. Radar measures<br />

an echo, which is influenced by type, size and c<strong>on</strong>centrati<strong>on</strong> of particles, all depending <strong>on</strong> the<br />

meteorological c<strong>on</strong>diti<strong>on</strong>s, ground clutter, shadowing by mountain ridges, attenuati<strong>on</strong> and<br />

parameters of the instrument itself. Calibrati<strong>on</strong> based directly <strong>on</strong> physical data is not possible,<br />

owing to the simple fact that no reliable data are available, since, as indicated above, rain gauge<br />

data are in error too. So <strong>on</strong>e tries to obtain the best possible agreement with point measurements,<br />

being aware, that neither the gauge value nor the <strong>radar</strong> interpretati<strong>on</strong> is necessarily correct.<br />

Therefore, <strong>radar</strong> is, and will be in future as well, a semi-quantitative measurement device.<br />

4<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005


MODULE A- INTRODUCTION TO RADAR<br />

2. RADAR THEORY<br />

2.1.The history of <strong>radar</strong><br />

Radar term is the abbreviati<strong>on</strong> of RAdio Detecti<strong>on</strong> And Ranging, i.e. finding and positi<strong>on</strong>ing a<br />

target and determining the distance between the target and the source by using radio frequency. This<br />

term was first used by the U.S. Navy in 1940 and adopted universally in 1943. It was originally<br />

called Radio Directi<strong>on</strong> Finding (R.D.F.) in England.<br />

We can say that, everything for <strong>radar</strong> started with the discovering of radio frequencies, and<br />

inventi<strong>on</strong> of some sub comp<strong>on</strong>ents, e.g. electr<strong>on</strong>ic devices, resulted inventi<strong>on</strong> and developing of<br />

<strong>radar</strong> <strong>systems</strong>. The history of <strong>radar</strong> includes the various practical and theoretical discoveries of the<br />

18 th , 19 th and early 20 th centuries that paved the way for the use of radio as means of<br />

communicati<strong>on</strong>. Although the development of <strong>radar</strong> as a stand-al<strong>on</strong>e technology did not occur until<br />

World War II, the basic principle of <strong>radar</strong> detecti<strong>on</strong> is almost as old as the subject of<br />

electromagnetism itself. Some of the major milest<strong>on</strong>es of <strong>radar</strong> history are as follows:<br />

• 1842 It was described by Christian Andreas Doppler that the sound waves from a<br />

source coming closer to a standing pers<strong>on</strong> have a higher frequency while the<br />

sound waves from a source going away from a standing pers<strong>on</strong> have a lower<br />

frequency. That approach is valid for radio waves, too. In other words, observed<br />

frequency of light and sound waves was affected by the relative moti<strong>on</strong> of the<br />

source and the detector. This phenomen<strong>on</strong> became known as the Doppler effect.<br />

• 1860 Electric and magnetic fields were discovered by Michael Faraday.<br />

• 1864 Mathematical equati<strong>on</strong>s of electromagnetism were determined by James Clark<br />

Maxwell. Maxwell set forth the theory of light must be accepted as an<br />

electromagnetic wave. Electromagnetic field and wave were put forth<br />

c<strong>on</strong>siderati<strong>on</strong> by Maxwell.<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005 5


MODULE A- INTRODUCTION TO RADAR<br />

• 1886 Theories of Maxwell were experimentally tested and similarity between radio<br />

and light waves was dem<strong>on</strong>strated by Heinrich Hertz.<br />

• 1888 Electromagnetic waves set forth by Maxwell were discovered by Heinrich Hertz.<br />

He showed that radio waves could be reflected by metallic and dielectric bodies.<br />

• 1900 Radar c<strong>on</strong>cept was documented by Nikola Tesla as “Exactly as the sound, so an<br />

electrical wave is reflected ... we may determine the relative positi<strong>on</strong> or <str<strong>on</strong>g>course</str<strong>on</strong>g><br />

of a moving object such as a vessel... or its speed."<br />

• 1904 The first patent of the detecti<strong>on</strong> of objects by radio was issued to Christian<br />

Hulsmayer (Figure-2.1)<br />

• 1922 Detecti<strong>on</strong> of ships by radio waves and radio communicati<strong>on</strong> between c<strong>on</strong>tinents<br />

was dem<strong>on</strong>strated by Gulielmo Marc<strong>on</strong>i.<br />

• 1922 A wooden ship was detected by using a CW <strong>radar</strong> by Albert Hoyt Taylor and<br />

Leo C.Young.<br />

• 1925 The first applicati<strong>on</strong> of the pulse technique was used to measure distance by G.<br />

Breit and M. Truve.<br />

• 1940 Microwaves were started to be used for l<strong>on</strong>g-range detecti<strong>on</strong>.<br />

• 1947 The first <strong>weather</strong> <strong>radar</strong> was installed in Washingt<strong>on</strong> D.C. <strong>on</strong> February 14.<br />

• 1950 Radars were put into operati<strong>on</strong> for the detecti<strong>on</strong> and tracking of <strong>weather</strong><br />

phenomena such as thunderstorms and cycl<strong>on</strong>es.<br />

• 1990’s A dramatic upgrade to <strong>radar</strong>s came in with the Doppler <strong>radar</strong>.<br />

6<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005


MODULE A- INTRODUCTION TO RADAR<br />

Figure-2.1 : First Radar Patent<br />

2.2. Basic Radar Terms<br />

It seems beneficial to give at least the definiti<strong>on</strong>s of some basic <strong>radar</strong> terms to be able to understand<br />

the theory and operati<strong>on</strong> of <strong>radar</strong>s. The comm<strong>on</strong> definiti<strong>on</strong>s of basic terms which will be talked<br />

about frequently during that <str<strong>on</strong>g>training</str<strong>on</strong>g> <str<strong>on</strong>g>course</str<strong>on</strong>g> are given below:<br />

a) Frequency (f)<br />

Frequency refers to the number of completed wave cycles per sec<strong>on</strong>d. Radar frequency is<br />

expressed in units of Hertz (Hz).<br />

b) Phase (δ )<br />

Phase of an electromagnetic wave is essentially the fracti<strong>on</strong> of a full wavelength a particular<br />

point is from some reference point measured in radians or degrees.<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005 7


MODULE A- INTRODUCTION TO RADAR<br />

c) Bandwidth (BW)<br />

The difference between the upper and lower frequencies of a band of electromagnetic<br />

radiati<strong>on</strong>.<br />

d) Wavelength ( λ )<br />

The distance from wave crest to wave crest (or trough to trough) al<strong>on</strong>g an electromagnetic<br />

wave’s directi<strong>on</strong> of travel is called wavelength.<br />

e) Pulse width (τ)<br />

Time interval between the leading edge and trailing edge of a pulse at a point where the<br />

amplitude is 50% of the peak value.<br />

f) PRF&PRT<br />

Pulse repetiti<strong>on</strong> frequency is the number of peak power pulses transmitted per sec<strong>on</strong>d.<br />

Pulse repetiti<strong>on</strong> time is the time interval between two peak pulses.<br />

g) Duty Factor/Duty Cycle<br />

Duty cycle is the amount of time a <strong>radar</strong> transmits compare to its listening or receiving time.<br />

The ratio is sometimes expressed in per cent. It can be determined by multiplying PRF and<br />

Pulse width or, by dividing the Pulse width with PRT.<br />

h) Beamwidth (θ)<br />

It is defined as the angle between the half-power (3 dB) points of the main lobe, when<br />

referenced to the peak effective radiated power of the main lobe<br />

Some Nomenclature<br />

Name Symbol Units Typical values<br />

transmitted frequency f t MHz, GHz 1000-12500 MHz<br />

wavelength λ cm 3-10 cm<br />

Pulse durati<strong>on</strong> τ µsec 1 µsec<br />

Pulse length h m 150-300 m (h=c τ)<br />

Pulse repetiti<strong>on</strong> frequency PRF sec -1 1000 sec -1<br />

interpulse period T millisec 1 millisec<br />

peak transmitted power P t MW 1 MW<br />

average power P avg kW 1 kW (Pavg = P t τ PRF)<br />

received power P r mW 10 -6 mW<br />

8<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005


MODULE A- INTRODUCTION TO RADAR<br />

2.3. Operati<strong>on</strong> Principle of Radar<br />

Operati<strong>on</strong> principle of a <strong>radar</strong> is very simple in theory and very similar to the way which bats use<br />

naturally to find their path during their flight (Figure-2.2). Bats use a type of <strong>radar</strong> system by<br />

emitting ultra-s<strong>on</strong>ic sounds in a certain frequency (120 KHz) and hearing the echoes of these<br />

sounds. These echoes make them enable to locate and avoid the objects in their path.<br />

Figure-2.2<br />

In the <strong>radar</strong> <strong>systems</strong>, an electromagnetic wave generated by the transmitter unit is transmitted by<br />

means of an antenna, and the reflected wave from the objects (echo) is received by the same<br />

antenna, and after processing of the returned signal a visual indicati<strong>on</strong> is displayed <strong>on</strong> indicators.<br />

After a radio signal is generated and emitted by a combinati<strong>on</strong> of a transmitter and an antenna, the<br />

radio waves travel out in a certain directi<strong>on</strong> in a manner similar to light or sound waves. If the<br />

signals strike an object, the waves are reflected and the reflected waves travel in all directi<strong>on</strong>s<br />

depending of the surface of the reflector. The term reflectivity refers to the amount of energy<br />

returned from an object and is dependent <strong>on</strong> the size, shape, and compositi<strong>on</strong> of the object. A small<br />

porti<strong>on</strong> of the reflected waves return to the locati<strong>on</strong> of the transmitter originating them where they<br />

are picked up by the receiver antenna. This signal is amplified and displayed <strong>on</strong> the screen of the<br />

indicators,e.g. PPI (Plan Positi<strong>on</strong> Indicator). This simple approach can be achieved by means of<br />

many complex process including hardware and software comp<strong>on</strong>ents.<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005 9


MODULE A- INTRODUCTION TO RADAR<br />

2.4. Radar Equati<strong>on</strong><br />

The fundamental relati<strong>on</strong> between the characteristics of the <strong>radar</strong>, the target, and the received signal<br />

is called the <strong>radar</strong> equati<strong>on</strong> and the theory of <strong>radar</strong> is developed based <strong>on</strong> that equati<strong>on</strong>.<br />

Pr<br />

=<br />

P<br />

t<br />

G<br />

2<br />

2<br />

θ H<br />

Π<br />

3<br />

K<br />

1024(ln2) λ<br />

2<br />

2<br />

L<br />

x<br />

Z<br />

R<br />

2<br />

This equati<strong>on</strong> involves variables that are either known or are directly measured. There is <strong>on</strong>ly <strong>on</strong>e<br />

value that is missing but it can be solved for mathematically. Below is the list of variables, what<br />

they are, and how they are measured.<br />

Pr: Average power returned to the <strong>radar</strong> from a target. The <strong>radar</strong> sends pulses and then measures<br />

the average power that is received in those returns. The <strong>radar</strong> uses multiple pulses since the power<br />

returned by a meteorological target varies from pulse to pulse. This is an unknown value of the<br />

<strong>radar</strong> but it is <strong>on</strong>e that is directly calculated.<br />

Pt: Peak power transmitted by the <strong>radar</strong>. This is a known value of the <strong>radar</strong>. It is important to know<br />

because the average power returned is directly related to the transmitted power.<br />

G: Antenna gain of the <strong>radar</strong>. This is a known value of the <strong>radar</strong>. This is a measure of the antenna's<br />

ability to focus outgoing energy into the beam. The power received from a given target is directly<br />

related to the square of the antenna gain.<br />

θ: Angular beam width of the <strong>radar</strong>. This is a known value of the <strong>radar</strong>. Through the Probert-J<strong>on</strong>es<br />

equati<strong>on</strong> it can be learned that the return power is directly related to the square of the angular beam<br />

width. The problem becomes that the assumpti<strong>on</strong> of the equati<strong>on</strong> is that precipitati<strong>on</strong> fills the beam<br />

for <strong>radar</strong>s with beams wider than two degrees. It is also an invalid assumpti<strong>on</strong> for any <strong>weather</strong> <strong>radar</strong><br />

at l<strong>on</strong>g distances. The lower resoluti<strong>on</strong> at great distances is called the aspect ratio problem.<br />

H: Pulse Length of the <strong>radar</strong>. This is a known value of the <strong>radar</strong>. The power received from a<br />

meteorological target is directly related to the pulse length.<br />

10<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005


MODULE A- INTRODUCTION TO RADAR<br />

K: This is a physical c<strong>on</strong>stant. This is a known value of the <strong>radar</strong>. This c<strong>on</strong>stant relies <strong>on</strong> the<br />

dielectric c<strong>on</strong>stant of water. This is an assumpti<strong>on</strong> that has to be made but also can cause some<br />

problems. The dielectric c<strong>on</strong>stant of water is near <strong>on</strong>e, meaning it has a good reflectivity. The<br />

problem occurs when you have meteorological targets that do not share that reflectivity. Some<br />

examples of this are snow and dry hail since their c<strong>on</strong>stants are around 0.2.<br />

L: This is the loss factor of the <strong>radar</strong>. This is a value that is calculated to compensate for attenuati<strong>on</strong><br />

by precipitati<strong>on</strong>, atmospheric gases, and receiver detecti<strong>on</strong> limitati<strong>on</strong>s. The attenuati<strong>on</strong> by<br />

precipitati<strong>on</strong> is a functi<strong>on</strong> of precipitati<strong>on</strong> intensity and wavelength. For atmospheric gases, it is a<br />

functi<strong>on</strong> of elevati<strong>on</strong> angle, range, and wavelength. Since all of these accounts for a 2dB loss, all<br />

signals are strengthened by 2 dB.<br />

λ: This is the wavelength of the transmitted energy. This is a known value of the <strong>radar</strong>. The amount<br />

of power returned from a precipitati<strong>on</strong> target is inversely since the short wavelengths are subject to<br />

significant attenuati<strong>on</strong>. The l<strong>on</strong>ger the wavelength, the less attenuati<strong>on</strong> caused by precipitate.<br />

Z: This is the reflectivity factor of the precipitate. This is the value that is solved for mathematically<br />

by the <strong>radar</strong>. The number of drops and the size of the drops affect this value. This value can cause<br />

problems because the <strong>radar</strong> cannot determine the size of the precipitate. The size is important since<br />

the reflectivity factor of a precipitati<strong>on</strong> target is determined by raising each drop diameter in the<br />

sample volume to the sixth power and then summing all those values together. A ¼" drop reflects<br />

the same amount of energy as 64 1/8" drops even though there is 729 times more liquid in the 1/8"<br />

drops.<br />

R: This is the target range of the precipitate. This value can be calculated by measuring the time it<br />

takes the signal to return. The range is important since the average power return from a target is<br />

inversely related to the square of its range from the <strong>radar</strong>. The <strong>radar</strong> has to normalize the power<br />

returned to compensate for the range attenuati<strong>on</strong>.<br />

Using a relati<strong>on</strong>ship between Z and R, an estimate of rainfall can be achieved. A base equati<strong>on</strong> that<br />

can be used to do this is Z=200*R 1.6 . This equati<strong>on</strong> can be modified at the user's request to a better<br />

fitting equati<strong>on</strong> for the day or the area.<br />

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2.4.1. How to derive <strong>radar</strong> equati<strong>on</strong><br />

It may be interesting for somebody so, a general derivati<strong>on</strong> steps of <strong>radar</strong> equati<strong>on</strong> is given below.<br />

Our starting point will be flux calculati<strong>on</strong>s.<br />

Flux Calculati<strong>on</strong>s - Isotropic Transmit<br />

Antenna<br />

Flux Calculati<strong>on</strong>s - Transmit Antenna with<br />

Gain<br />

Figure -2.3: Flux at distance R<br />

Figure-2.4: Flux at distance R with gain.<br />

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Radar Signal @ Target, Incident power flux density from a Directive Source<br />

Figure-2.5: Incident power flux density from a Directive Source.<br />

Echo Signal @ Target, Backscattered power from the target<br />

Figure-2.6: Power back scattered from target with cross secti<strong>on</strong>.<br />

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Target Echo @ Radar Backscattered power flux at the <strong>radar</strong><br />

Figure-2.7: Flux back scattered from target at <strong>radar</strong>.<br />

Radar Cross Secti<strong>on</strong><br />

The <strong>radar</strong> cross secti<strong>on</strong> (σ) of a target is the “equivalent area” of a flat-plate mirror:<br />

♦<br />

♦<br />

That is aligned perpendicular to the propagati<strong>on</strong> directi<strong>on</strong> (i.e., reflects the signal directly<br />

back to the transmitter) and<br />

That results in the same backscattered power as produced by the target<br />

Radar cross secti<strong>on</strong> is extremely difficult to predict and is usually measured using scaled models<br />

of targets<br />

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Target Echo Signal @ Radar Received (echo) power at the <strong>radar</strong><br />

Figure -2.8: Received power at <strong>radar</strong>.<br />

Relati<strong>on</strong>ship between Antenna Aperture and Gain<br />

Figure -2.9: Antenna aperture and gain.<br />

Where A= the physical aperture area of the antenna<br />

ρ a<br />

=the aperture collecti<strong>on</strong> efficiency<br />

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λ= the electromagnetic wave length<br />

Idealized Radar Equati<strong>on</strong> - no system losses<br />

Since the antenna gain is the same for transmit & receive, this becomes :<br />

Practical Radar Equati<strong>on</strong> - with system losses for point targets<br />

Where:<br />

• Lsys = the system losses expressed as a power ratio<br />

• P r is the average received power<br />

• P t is the transmitted power<br />

• G is the gain for the <strong>radar</strong><br />

• λ is the <strong>radar</strong>'s wavelength<br />

• σ is the targets scattering cross secti<strong>on</strong><br />

• R is the range from the <strong>radar</strong> to the target<br />

• L sys: is system losses.<br />

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The <strong>radar</strong> equati<strong>on</strong> for a point target is simply given below:<br />

Radar Equati<strong>on</strong> For Distributed Targets<br />

Thus far, we've derived the <strong>radar</strong> equati<strong>on</strong> for a point target. This is enough if you are interested<br />

in point targets such as airplanes. However, in a thunderstorm or some area of precipitati<strong>on</strong>, we<br />

do not have just <strong>on</strong>e target (e.g., raindrop), we have many. Thus we need to derive the <strong>radar</strong><br />

equati<strong>on</strong> for distributed targets. So let’s review the Radar Pulse Volume.<br />

Radar Pulse Volume<br />

First, let's simplify the real beam according to the Figure 1.2.15:<br />

Figure -2.10: Radar pulses<br />

What does a "three-dimensi<strong>on</strong>al" segment of the <strong>radar</strong> beam look like<br />

Figure -2.11: Radar main beam and pulse volume.<br />

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Figure -2.12: Form of transmit and received signal.<br />

So, the “volume” of the pulse volume is:<br />

For a circular beam, then θ=Φ, the pulse volume becomes:<br />

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Before we derive the <strong>radar</strong> equati<strong>on</strong> for the distributed targets situati<strong>on</strong>, we need to make some<br />

assumpti<strong>on</strong>s:<br />

1) The beam is filled with targets.<br />

2) Multiple scattering is ignored<br />

3) Total average power is equal to sum of powers scattered by individual particles.<br />

Recall the <strong>radar</strong> equati<strong>on</strong> for a single target:<br />

(1)<br />

For multiple targets, <strong>radar</strong> equati<strong>on</strong> (1) can be written as:<br />

(2)<br />

where the sum is over all targets within the pulse volume.<br />

If we assume that h/2


MODULE A- INTRODUCTION TO RADAR<br />

Thus, (5) can be written as:<br />

(5)<br />

Substituting (5) into (3) gives:<br />

(6)<br />

Note that:<br />

P r is proporti<strong>on</strong>al to R -2 for distributed targets.<br />

P r is proporti<strong>on</strong>al to R -4 for point targets.<br />

Radar Reflectivity<br />

The sum of all backscattering cross secti<strong>on</strong>s (per unit volume) is referred to as the <strong>radar</strong><br />

reflectivity (η). In other words,<br />

(7)<br />

In terms of the <strong>radar</strong> reflectivity, the <strong>radar</strong> equati<strong>on</strong> for distributed targets (21) can be written as:<br />

(8)<br />

All variables in (8), except η are either known or measured.<br />

Now, we need to add a fudge factor due to the fact that the beam shape is Gaussian.<br />

Hence, (8) becomes;<br />

(9)<br />

Complex Dielectric Factor<br />

The backscattering cross secti<strong>on</strong> (σ i ) can be written as:<br />

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(10)<br />

Where:<br />

• D is the diameter of the target<br />

• λ is the wavelength of the <strong>radar</strong><br />

• Kis the complex dielectric factor<br />

o<br />

is some indicati<strong>on</strong> of how good a material is at backscattering radiati<strong>on</strong><br />

For water =0.93<br />

For ice =0.197<br />

Notice that the value for water is much larger than for ice. All other factors the same, this creates<br />

a 5dB difference in returned power<br />

So, let's incorporate this informati<strong>on</strong> into the <strong>radar</strong> equati<strong>on</strong>.<br />

Recall from (22) that .<br />

Using (11) can be written<br />

as:<br />

(12)<br />

Taking the c<strong>on</strong>stants out of the sum;<br />

(13)<br />

Remember that the sum is for a unit volume. Substituting (27) into (24) gives:<br />

(14)<br />

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Simplifying terms gives:<br />

P<br />

r<br />

=<br />

PG<br />

t<br />

2<br />

2<br />

3<br />

θ π h K<br />

2<br />

1024ln 2R<br />

λ<br />

2<br />

2<br />

∑<br />

i<br />

D<br />

6<br />

i<br />

(15)<br />

Note the D i 6 dependence <strong>on</strong> the average received power.<br />

Radar Reflectivity Factor<br />

In Equati<strong>on</strong> (15), all variables except the summati<strong>on</strong> term, are either known or measured.<br />

We will now define the <strong>radar</strong> reflectivity factor, Z as:<br />

(16)<br />

Substituting (30) into (29) gives the <strong>radar</strong> equati<strong>on</strong> for distributed targets:<br />

P<br />

r<br />

=<br />

P G<br />

t<br />

2<br />

θ<br />

2<br />

3<br />

π h K<br />

2<br />

1024ln 2λ<br />

R<br />

2<br />

2<br />

Z<br />

(17)<br />

• Note the relati<strong>on</strong>ship between the received power, range and <strong>radar</strong> wavelength<br />

• Everything in Equati<strong>on</strong> (17) is measured or known except Z, the <strong>radar</strong> reflectivity factor.<br />

• Since the strength of the received power can span many orders of magnitude, then so<br />

does Z.<br />

• Hence, we take the log <strong>on</strong> Z according to:<br />

(18)<br />

• The dBZ value calculated above is what you see displayed <strong>on</strong> the <strong>radar</strong> screen or <strong>on</strong><br />

imagery accessed from the web.<br />

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As a result, formulas can be written as follows:<br />

! Point target <strong>radar</strong> equati<strong>on</strong>:<br />

p<br />

r<br />

p g<br />

λ A<br />

2 2<br />

t<br />

3<br />

64π<br />

r<br />

σ<br />

4<br />

=<br />

( )<br />

2<br />

! Meteorological target <strong>radar</strong> equati<strong>on</strong><br />

p<br />

r<br />

5 2<br />

π pt<br />

g θφτ c K<br />

=<br />

2<br />

1024ln2λ<br />

r<br />

2<br />

zl<br />

2.5. Block Diagram of A Radar<br />

Radar <strong>systems</strong>, like other complex electr<strong>on</strong>ics <strong>systems</strong>, are composed of several major<br />

sub<strong>systems</strong> and many individual circuits. Although modern <strong>radar</strong> <strong>systems</strong> are quite complicated,<br />

you can easily understand their operati<strong>on</strong> by using a basic <strong>radar</strong> block diagram.<br />

The Figure -2.14 below shows us the basic <strong>radar</strong> block diagram.<br />

Figure -2.14: Basic Radar Diagram<br />

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The parts of this block diagram in Figure-2.14. are described below:<br />

Master Clock/Computer: In older <strong>radar</strong>s, this device was called the master clock. It would<br />

generate all of the appropriate signals and send them to the appropriate comp<strong>on</strong>ents of the <strong>radar</strong>.<br />

In modern <strong>radar</strong>s, the functi<strong>on</strong> of the master clock has been taken over by the ubiquitous<br />

computer. Computers now c<strong>on</strong>trol <strong>radar</strong>s just as they c<strong>on</strong>trol many other parts of modern<br />

technology.<br />

Transmitter: The source of the EM radiati<strong>on</strong> emitted by a <strong>radar</strong> is the transmitter. It generates<br />

the high frequency signal which leaves the <strong>radar</strong>’s antenna and goes out into the atmosphere. The<br />

transmitter generates powerful pulses of electromagnetic energy at precise intervals. The<br />

required power is obtained by using a high-power microwave oscillator (such as a magnetr<strong>on</strong>) or<br />

a microwave amplifier (such as a klystr<strong>on</strong>) that is supplied by a low- power RF source.<br />

Modulator: The purpose of modulator is to switch the transmitter <strong>on</strong> and off and to provide the<br />

correct waveform for the transmitted pulse. That is, the modulator tells the transmitter when to<br />

transmit and for what durati<strong>on</strong>.<br />

Waveguide: Figure 1.2.6 shows that the c<strong>on</strong>necting the transmitter and the antenna is<br />

waveguide. This is usually a hollow, rectangular, metal c<strong>on</strong>ductor whose interior dimensi<strong>on</strong>s<br />

depend up<strong>on</strong> the wavelength of the signals being carried. Waveguide is put together much like<br />

the copper plumbing in a house. L<strong>on</strong>g piece of waveguide are c<strong>on</strong>nected together by special<br />

joints to c<strong>on</strong>nect the transmitter/receiver and the antenna.<br />

Antenna: The antennas are the device which sends the <strong>radar</strong>’s signal into atmosphere. Most<br />

antennas used with <strong>radar</strong>s are directi<strong>on</strong>al; that is, they focus the energy into a particular directi<strong>on</strong><br />

and not other directi<strong>on</strong>s. An antenna that sends radiati<strong>on</strong> equally in all directi<strong>on</strong>s is called<br />

isotropic antenna.<br />

Receiver: The receiver is designed to detect and amplify the very weak signals received by<br />

antenna. Radar receivers must be of very high quality because the signals that are detected are<br />

often very weak.<br />

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Display: There are many way to display <strong>radar</strong> data. The earliest and easiest display for <strong>radar</strong><br />

data was to put it <strong>on</strong>to a simple oscilloscope. After that A-scope was found. PPI and RHI are<br />

new techniques for displaying the <strong>radar</strong> data.<br />

Duplexer: Duplexer, somebody called Transmit/receive switch, is a special switch added to the<br />

<strong>radar</strong> system to protect the receiver from high power of the transmitter.<br />

Of <str<strong>on</strong>g>course</str<strong>on</strong>g> this is a briefly explanati<strong>on</strong> about comp<strong>on</strong>ents of a <strong>radar</strong>. Later <strong>on</strong> this <str<strong>on</strong>g>course</str<strong>on</strong>g>, besides<br />

these parts, all comp<strong>on</strong>ents will be explained in detail. Figure 2.15 shows us some important<br />

comp<strong>on</strong>ents of a <strong>radar</strong>.<br />

Figure -2.15: Block diagram of a <strong>radar</strong>.<br />

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3. PROPOGATION OF EM WAVES<br />

Radar signals are emitted in some frequencies within the electromagnetic spectrum located in a<br />

range from a few MHz to 600 GHz. First let us review the electromagnetic spectrum.<br />

3. 1. Electromagnetic Spectrum<br />

All things (which have temperature above absolute zero) emit radiati<strong>on</strong>. Radiati<strong>on</strong> is energy that<br />

travels in the form of waves. Since radiati<strong>on</strong> waves have electrical and magnetic properties, they<br />

are called as “electromagnetic waves”.<br />

Most of the electromagnetic energy <strong>on</strong> the earth originates from the sun. The sun actually<br />

radiates electromagnetic energy at several different wavelengths and frequencies, ranging from<br />

gamma rays to radio waves. Collectively, these wavelengths and frequencies make up the<br />

electromagnetic spectrum.<br />

Figure -3.1<br />

Frequency and wavelength of electromagnetic waves change with inverse of other. According to<br />

the famous formula about light, then f can be calculated as follows:<br />

λ=c/f " f= c/λ " T = 1 / f [s] " λ = c/f = 299,792,458 / f [m] (f in Hz [s -1 ])<br />

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Figure-3.2: The relati<strong>on</strong> between frequency and wavelength<br />

A <strong>radar</strong> operates in microwave regi<strong>on</strong> of EM spectrum and it emits the energy in the form of EM<br />

wave into the atmosphere through an antenna. While <strong>on</strong>ly a fragment of the energy returns, it<br />

provides a great deal of informati<strong>on</strong>. The entire process of energy propagating through space,<br />

striking objects, and returning occurs at the speed of light. Targets are struck by electromagnetic<br />

energy and the return signals from these targets are called <strong>radar</strong> echoes.<br />

The table below shows the electromagnetic spectrum and the locati<strong>on</strong> of <strong>radar</strong> frequencies<br />

in that spectrum.<br />

Figure-3.3<br />

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The <strong>radar</strong> bands located in the spectrum have been designated by certain letters as follows:<br />

Band Designati<strong>on</strong> Nominal Frequency Nominal Wavelength<br />

HF 3-30 MHz 100-10 m<br />

VHF 30-300 MHz 10-1 m<br />

UHF 300-1000 MHz 1-0.3 m<br />

L 1-2 GHz 30-15 cm<br />

S 2-4 GHz 15-8 cm<br />

C 4-8 GHz 8-4 cm<br />

X 8-12 GHz 4-2.5 cm<br />

Ku 12-18 GHz 2.5-1.7 cm<br />

K 18-27 GHz 1.7-1.2 cm<br />

Ka 27-40 GHz 1.2-0.75 cm<br />

V 40-75 GHz 0.75-0.40 cm<br />

W 75-110 GHz 0.40-0.27 cm<br />

mm 110-300 GHz 0.27-0.1 cm<br />

Specific frequencies within above ranges have been assigned for <strong>radar</strong>s by Internati<strong>on</strong>al<br />

Telecommunicati<strong>on</strong> Uni<strong>on</strong> (ITU). The radio frequency bands used by <strong>weather</strong> <strong>radar</strong>s are located<br />

around 2.8 GHz (S-Band), 5.6 GHz (C-Band), 9.4 GHz (X-Band) and 35.6 GHz (Ka-Band).<br />

3. 2. Electromagnetic waves<br />

Electromagnetic or radio waves c<strong>on</strong>sist of electric (E) and magnetic (H) force fields, which are<br />

perpendicular to each other and to the directi<strong>on</strong> of propagati<strong>on</strong> of the wave fr<strong>on</strong>t, propagate<br />

through space at the speed of light and interact with matter al<strong>on</strong>g their paths. These waves have<br />

sinusoidal spatial and temporal variati<strong>on</strong>s. The distance or time between successive wave peaks<br />

(or other reference points) of the electric (magnetic) force defines the wavelength λ or wave<br />

period T. These two important electromagnetic field parameters are related to the speed of light<br />

c. The wave period T is the reciprocal of the frequency f. Frequency refers to the number of<br />

completed wave cycles per sec<strong>on</strong>d. Radar frequency is expressed in units of Hertz (Hz). Higher<br />

frequency transmitters produce shorter wavelengths and vice versa. Wave amplitude is simply<br />

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the wave’s height (from the midline positi<strong>on</strong>) and represents the amount of energy c<strong>on</strong>tained<br />

within the wave.<br />

Figure-3.4<br />

3.2.1. Polarizati<strong>on</strong><br />

As menti<strong>on</strong>ed previously, electromagnetic radiati<strong>on</strong> c<strong>on</strong>sists of electric and magnetic fields<br />

which oscillate with the frequency of radiati<strong>on</strong>. These fields are always perpendicular to each<br />

other. So, it is possible to specify the orientati<strong>on</strong> of the electromagnetic radiati<strong>on</strong> by specifying<br />

the orientati<strong>on</strong> of <strong>on</strong>e of those fields. The orientati<strong>on</strong> of the electric field is defined as the<br />

orientati<strong>on</strong> of electromagnetic field and this is called as “polarizati<strong>on</strong>”. In other words,<br />

polarizati<strong>on</strong> refers to the orientati<strong>on</strong> of the electrical field comp<strong>on</strong>ent of an electromagnetic<br />

wave.<br />

The plane of polarisati<strong>on</strong> c<strong>on</strong>tains both the electric vector and the directi<strong>on</strong> of propagati<strong>on</strong>.<br />

Simply because the plane is two-dimensi<strong>on</strong>al, the electric vector in the plane at a point in space<br />

can be decomposed into two orthog<strong>on</strong>al comp<strong>on</strong>ents. Call these the x and y comp<strong>on</strong>ents<br />

(following the c<strong>on</strong>venti<strong>on</strong>s of analytic geometry). For a simple harm<strong>on</strong>ic wave, where the<br />

amplitude of the electric vector varies in a sinusoidal manner, the two comp<strong>on</strong>ents have exactly<br />

the same frequency. However, these comp<strong>on</strong>ents have two other defining characteristics that can<br />

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differ. First, the two comp<strong>on</strong>ents may not have the same amplitude. Sec<strong>on</strong>d, the two comp<strong>on</strong>ents<br />

may not have the same phase that is they may not reach their maxima and minima at the same<br />

time in the fixed plane we are talking about. By c<strong>on</strong>sidering the shape traced out in a fixed plane<br />

by the electric vector as such a plane wave passes over it, we obtain a descripti<strong>on</strong> of the<br />

polarizati<strong>on</strong> state. By c<strong>on</strong>sidering that issue, three types of polarizati<strong>on</strong> of electromagnetic<br />

waves can be defined. These are Linear, Circular and Elliptical Polarizati<strong>on</strong>s.<br />

a) Linear polarizati<strong>on</strong><br />

If the electrical vector remains in <strong>on</strong>e plane, then the wave is linearly polarised. By c<strong>on</strong>venti<strong>on</strong>,<br />

if the electric vector (or field) is parallel to the earth's surface, the wave is said to be horiz<strong>on</strong>tally<br />

polarized, if the electric vector (or field) is perpendicular to the earth's surface, the wave is said to<br />

be vertically polarized.<br />

Linear polarizati<strong>on</strong> is shown in Figure-3.5. Here, two oorthog<strong>on</strong>al comp<strong>on</strong>ents (Ex-red and Eygreen)<br />

of the electric field vector (E-blue) are in phase and they form a path (purple) in the<br />

plane while propagating. In linear polarizati<strong>on</strong> case, the strength of the two comp<strong>on</strong>ents are<br />

always equal or related by a c<strong>on</strong>stant ratio, so the directi<strong>on</strong> of the electric vector (the vector sum<br />

of these two comp<strong>on</strong>ents) will always fall <strong>on</strong> a single line in the plane. We call this special case<br />

linear polarizati<strong>on</strong>. The directi<strong>on</strong> of this line will depend <strong>on</strong> the relative amplitude of the two<br />

comp<strong>on</strong>ents. This directi<strong>on</strong> can be in any angle in the plane, but the directi<strong>on</strong> never varies.<br />

Linear polarisati<strong>on</strong> is most often used in c<strong>on</strong>venti<strong>on</strong>al <strong>radar</strong> antennas since it is the easiest to<br />

achieve. The choice between horiz<strong>on</strong>tal and vertical polarisati<strong>on</strong> is often left to the discreti<strong>on</strong> of<br />

the antenna designer, although the <strong>radar</strong> system engineer might sometimes want to specify <strong>on</strong>e or<br />

the other, depending up<strong>on</strong> the importance of ground reflecti<strong>on</strong>s.<br />

Figure-3.5<br />

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b) Circular polarizati<strong>on</strong><br />

In case of circular polarizati<strong>on</strong> as shown in Figure-3.6, the two orthog<strong>on</strong>al comp<strong>on</strong>ents (Ex-red<br />

and Ey-green) of the electric field vector (E-blue) have exactly the same amplitude and are<br />

exactly ninety degrees out of phase and they form a path (purple) in the plane while<br />

propagating. In this case, <strong>on</strong>e comp<strong>on</strong>ent is zero when the other comp<strong>on</strong>ent is at maximum or<br />

minimum amplitude. Notice that there are two possible phase relati<strong>on</strong>ships that satisfy this<br />

requirement. The x comp<strong>on</strong>ent can be ninety degrees ahead of the y comp<strong>on</strong>ent or it can be<br />

ninety degrees behind the y comp<strong>on</strong>ent. In this special case the electrical vector will be rotating<br />

in a circle while the wave propagates. The directi<strong>on</strong> of rotati<strong>on</strong> will depend <strong>on</strong> which of the two<br />

phase relati<strong>on</strong>ships exists.One rotati<strong>on</strong> is finished after <strong>on</strong>e wavelength. The rotati<strong>on</strong> may be left<br />

or right handed. In other words, image of the electric field vector (E) will be circular and<br />

electromagnetic wave will be circularly polarized. Circular polarisati<strong>on</strong> is often desirable to<br />

attenuate the reflecti<strong>on</strong>s of rain with respect to aircraft.<br />

Figure-3.6<br />

c) Elliptical polarizati<strong>on</strong><br />

As shown in Figure 3.7, two comp<strong>on</strong>ents (Ex-red and Ey-green) of the electric field vector (Eblue)<br />

are not in phase and either do not have the same amplitude and/or are not ninety degrees<br />

out of phase. So the path (purple) formed in the plane while propagating will trace out an ellipse<br />

and this is called as elliptical polarizati<strong>on</strong>. In other words, image of electric field vector E will<br />

be elliptical and electromagnetic wave will be elliptically polarized. In fact linear and circular<br />

polarizati<strong>on</strong>s are special cases of the elliptical polarizati<strong>on</strong>.<br />

Figure-3.7<br />

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3.3. Refracti<strong>on</strong><br />

Electromagnetic waves propagating within the earth's atmosphere do not travel in straight lines<br />

but are generally refracted. The density differences in the atmosphere affect the speed and<br />

directi<strong>on</strong> of electromagnetic waves. In some regi<strong>on</strong>s, a wave may speed up, while in other<br />

regi<strong>on</strong>s it may slow down. This situati<strong>on</strong> is known as refracti<strong>on</strong>. One effect of refracti<strong>on</strong> is to<br />

extend the distance to the horiz<strong>on</strong>, thus increasing the <strong>radar</strong> coverage. Another effect is the<br />

introducti<strong>on</strong> of errors in the measurement of the elevati<strong>on</strong> angle. Refracti<strong>on</strong> of the <strong>radar</strong> waves in<br />

the atmosphere is caused by the variati<strong>on</strong> with altitude of the velocity of propagati<strong>on</strong>, or the<br />

index of refracti<strong>on</strong>, defined as the velocity of propagati<strong>on</strong> in free space to that in the medium in<br />

questi<strong>on</strong>. Now, let us remind some basic parameters regarding refracti<strong>on</strong>.<br />

Refracti<strong>on</strong> Models<br />

N<strong>on</strong>-standard refracti<strong>on</strong> model<br />

(1992)<br />

Figure-3.8<br />

Doviak and Zrnic 2002<br />

3.3.1. Refractive index<br />

The speed of electromagnetic radiati<strong>on</strong> depends up<strong>on</strong> the material through which it is travelling.<br />

In a vacuum such as the nearly empty space between the sun and earth, for example, light travels<br />

at a speed of 299 792 458 ± 6 m/s, according to the Nati<strong>on</strong>al Bureau of Standards (Cohen and<br />

Taylor,1987)<br />

When electromagnetic radiati<strong>on</strong> travels through air or other materials, it travels slightly slower<br />

than in a vacuum. The ratio of the speed of light in a vacuum to the speed of light in a medium is<br />

called the refractive index of the medium and is defined mathematically as<br />

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n=c/u<br />

where c is the speed of light in a vacuum, u is the speed of the light in the medium and n is the<br />

refractive index.<br />

The refractive index of the atmosphere depends up<strong>on</strong> atmospheric pressure, temperature and<br />

vapour pressure. Although the number of free electr<strong>on</strong>s present also affects the refractivity of the<br />

atmosphere, this can be ignored in troposphere due to insufficient free electr<strong>on</strong>s. At microwave<br />

frequencies, the index of refracti<strong>on</strong> n for air which c<strong>on</strong>tains water vapour is<br />

77.6 p 3.73e10<br />

(n-1)10 6 =N= +<br />

2<br />

T T<br />

5<br />

where p = barometric pressure in hPa, e = partial pressure of water vapour in hPa, and T = absolute<br />

temperature in K. The parameter N is called refractivity. N is defined as follows:<br />

N=(n-1) 10 6<br />

If n=1.0003 then N will be 300.<br />

These values may be gathered by radios<strong>on</strong>des. The index of refracti<strong>on</strong> normally decreases with<br />

increasing altitude and is typically 1.000313 near the surface of the earth, i.e. N = 313. This means<br />

that electromagnetic radiati<strong>on</strong> travels approximately 0.0313 % slower there than in a vacuum.<br />

3.3.2. Curvature<br />

Curvature is defined as “the rate of change in the deviati<strong>on</strong> of a given arc from any tangent to it.”<br />

Stated another way, it is the angular rate of change necessary to follow a curved path. Another<br />

definiti<strong>on</strong> of curvature is the reciprocal of the radius and expressed as follows:<br />

C= δθ/ δS<br />

Where δθ is the change in angle experienced over a distance δS. When we think about a circle<br />

with a radius of R, expressi<strong>on</strong> becomes;<br />

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C= δθ/ δS = 2π/2πR=1/R<br />

For a <strong>radar</strong> ray travelling relative to the earth when there is a n<strong>on</strong>-uniform atmosphere present,<br />

the ray will bend more or less relative to the earth, depending up<strong>on</strong> how much the refractive<br />

index changes with height. Then;<br />

C= δθ/ δS=1/R + δn/ δH<br />

It is sometimes c<strong>on</strong>venient to think of the <strong>radar</strong> rays travelling in straight lines instead of the<br />

actual curved paths they do follow. We can accomplish this by creating a fictitious earth radius is<br />

different from the true earth’s radius. This effective earth’s radius R’ is given by<br />

1/R’=1/R + δn/ δH<br />

There are various relati<strong>on</strong>ships between curvature, earth’s radius, effective earth’s radius, and<br />

refractive index gradient. So it is possible to calculate the actual path a <strong>radar</strong> ray will follow in<br />

real atmospheric c<strong>on</strong>diti<strong>on</strong>s.<br />

4. RADAR TYPES<br />

Radars may be classified in several ways due to the criteria of the classificati<strong>on</strong>, e.g. receiving<br />

and transmitting type, purpose of the use, operating frequency band, signal emitting type (pulse-<br />

CW), polarizati<strong>on</strong> type. It is also possible to make sub classificati<strong>on</strong>s under the main<br />

classificati<strong>on</strong> of <strong>radar</strong>s. So major types of <strong>radar</strong>s have been denominated as m<strong>on</strong>ostatic, bistatic,<br />

pulse, c<strong>on</strong>tinuous (CW), Doppler, n<strong>on</strong>-Doppler, <strong>weather</strong> <strong>radar</strong>, air surveillance <strong>radar</strong>, mobile<br />

<strong>radar</strong>, stati<strong>on</strong>ary <strong>radar</strong>, X-Band, L-Band, C-Band, S-Band, K-Band, single polarizati<strong>on</strong> <strong>radar</strong>s,<br />

polarimetric <strong>radar</strong>s, etc. Although our main c<strong>on</strong>cern is Doppler <strong>weather</strong> <strong>radar</strong>s which will be<br />

studied in detail, some brief explanati<strong>on</strong> of major types of the <strong>radar</strong>s are also given below:<br />

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4.1. M<strong>on</strong>ostatic Radars<br />

M<strong>on</strong>ostatic <strong>radar</strong>s use a comm<strong>on</strong> or adjacent antennas for transmissi<strong>on</strong> and recepti<strong>on</strong>, where the<br />

<strong>radar</strong>s receiving antenna is in relati<strong>on</strong>ship to its transmitting antenna. Most <strong>radar</strong> system are use<br />

a single antenna for both transmitting and receiving; the received signal must come back to the<br />

same place it left in order to be received. This kind of <strong>radar</strong> is a m<strong>on</strong>ostatic <strong>radar</strong>. Doppler<br />

<strong>weather</strong> <strong>radar</strong>s are m<strong>on</strong>ostatic <strong>radar</strong>s.<br />

4.2. Bistatic Radars<br />

A bistatic <strong>radar</strong> has two antennas. Sometimes these are side by side, but sometimes the<br />

transmitter and its antenna at <strong>on</strong>e locati<strong>on</strong> and the receiver and its antenna at another. In this kind<br />

of <strong>radar</strong> the transmitting <strong>radar</strong> system aims at a particular place in the sky where a cloud or other<br />

target is located. The signal from this point is scattered or reradiated in many directi<strong>on</strong>s, much of<br />

being in a generally forward directi<strong>on</strong>. Such receiving <strong>systems</strong> may also be called passive <strong>radar</strong><br />

<strong>systems</strong>.<br />

4.3. Air Surveillance Radars (ASR)<br />

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The ASR system c<strong>on</strong>sists of two sub<strong>systems</strong>: primary surveillance <strong>radar</strong> and sec<strong>on</strong>dary<br />

surveillance <strong>radar</strong>. The primary surveillance <strong>radar</strong> uses a c<strong>on</strong>tinually rotating antenna mounted<br />

<strong>on</strong> a tower to transmit electromagnetic waves, which reflect from the surface of aircraft up to 60<br />

nautical miles from the <strong>radar</strong>. The <strong>radar</strong> system measures the time required for the <strong>radar</strong> echo to<br />

return and the directi<strong>on</strong> of the signal. From this data, the system can measure the distance of the<br />

aircraft from the <strong>radar</strong> antenna and the azimuth or directi<strong>on</strong> of the aircraft from the antenna. The<br />

primary <strong>radar</strong> also provides data <strong>on</strong> six levels of rainfall intensity. The primary <strong>radar</strong> operates in<br />

the range of 2700 to 2900 MHz.<br />

The sec<strong>on</strong>dary <strong>radar</strong>, also called as the beac<strong>on</strong> <strong>radar</strong>, uses a sec<strong>on</strong>d <strong>radar</strong> antenna attached to the<br />

top of the primary <strong>radar</strong> antenna to transmit and receive aircraft data such as barometric altitude,<br />

identificati<strong>on</strong> code, and emergency c<strong>on</strong>diti<strong>on</strong>s. Military and commercial aircraft have<br />

transp<strong>on</strong>ders that automatically resp<strong>on</strong>d to a signal from the sec<strong>on</strong>dary <strong>radar</strong> with an<br />

identificati<strong>on</strong> code and altitude.<br />

4.4. 3D Radars<br />

A three-dimensi<strong>on</strong>al <strong>radar</strong> is capable of producing three-dimensi<strong>on</strong>al positi<strong>on</strong> data <strong>on</strong> a<br />

multiplicity of targets (range, azimuth, and height). There are several ways to achieve 3D data. A<br />

2D <strong>radar</strong> just provides azimuth and range informati<strong>on</strong>.<br />

4.5. Senthetic Aperture Radars<br />

SAR are being used in air and space-borne <strong>systems</strong> for remote sensing. The inherent high<br />

resoluti<strong>on</strong> of this <strong>radar</strong> type is achieved by a very small beam width which in turn is generated by<br />

an effective l<strong>on</strong>g antenna, namely by signal-processing means rather by the actual use of a l<strong>on</strong>g<br />

physical antenna. This is d<strong>on</strong>e by moving a single radiating line of elements mounted e.g. in an<br />

aircraft and storing the received signals to form the target picture afterwards by signal<br />

processing. The resulting <strong>radar</strong> images look like photos because of the high resoluti<strong>on</strong>. Instead of<br />

moving a <strong>radar</strong> relatively to a stati<strong>on</strong>ary target, it is possible to generate an image by moving the<br />

object relative to a stati<strong>on</strong>ary <strong>radar</strong>. This method is called Inverse SAR (ISAR) or range Doppler<br />

imaging.<br />

4.6. C<strong>on</strong>tinuous Wave (CW) Radars<br />

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The CW transmitter generates c<strong>on</strong>tinuously unmodulated RF waves of c<strong>on</strong>stant frequency<br />

which pass the antenna and travel through the space until they are reflected by an object.<br />

The isolator shall prevent any direct leakage of the transmitter energy into the receiver and<br />

thus avoid the saturati<strong>on</strong> or desensitisati<strong>on</strong> of the receiver which must amplify the small<br />

signals received by the antenna. The CW <strong>radar</strong> can <strong>on</strong>ly detect the presence of a reflected<br />

object and its directi<strong>on</strong> , but it cannot extract range for there are no c<strong>on</strong>venient time marks in<br />

which to measure the time interval. Therefore this <strong>radar</strong> is used mainly to extract the speed<br />

of moving objects. The principle used is the Doppler effect. The Doppler principle will be<br />

explained in detail in following chapters.<br />

4.7 FM-CW Radars<br />

The inability of a simple CW <strong>radar</strong> to measure range is related to the relatively narrow spectrum<br />

(bandwidth) of its transmitted waveform. Some sort of timing mark must be applied to the CW<br />

carrier if range is to be measured. The timing mark permits the time of transmissi<strong>on</strong> and the time<br />

of return to be recognised. The sharper or more distinct the mark, the more accurate is the<br />

measurement of the transit time. But the more distinct the timing mark, the broader will be the<br />

transmitted spectrum. Therefore a certain spectrum width must be transmitted if transit time or<br />

range is to be measured.<br />

The spectrum of a CW transmissi<strong>on</strong> can be broadened by the applicati<strong>on</strong> of modulati<strong>on</strong>, either by<br />

modulating the amplitude, the frequency, or the phase. An example of the amplitude modulati<strong>on</strong><br />

is the pulse <strong>radar</strong>.<br />

4.8. Moving Target Indicati<strong>on</strong> (MTI) Radars<br />

The purpose of MTI <strong>radar</strong> is to reject signals from fixed unwanted signals, sky and/or ground<br />

clutter, and retain for detecti<strong>on</strong> the signals from moving targets such as aircraft or rain. There are<br />

two basic types of MTI namely coherent and n<strong>on</strong>-coherent MTI. The former utilises the Doppler<br />

shift imparted <strong>on</strong> the reflected signal by a moving target to distinguish moving targets from fixed<br />

targets, and the latter detects moving targets by the relative moti<strong>on</strong> between the target and an<br />

extended clutter background and c<strong>on</strong>sequently by the corresp<strong>on</strong>ding amplitude changes from<br />

pulse to pulse or from <strong>on</strong>e antenna scan to the next. By coherent it is meant that the phase of the<br />

transmitted wave must be preserved for use by the receiver if the Doppler shift in frequency is to<br />

be detected, whereas in n<strong>on</strong>-coherent <strong>systems</strong> it is not necessary.<br />

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4.9. Pulse Radars<br />

Pulse <strong>radar</strong> is a primary <strong>radar</strong> unit which transmits a high-frequency impulsive signal of high<br />

power. After this a l<strong>on</strong>ger break in which the echoes can be received follows before a new<br />

transmitted signal is sent out. Directi<strong>on</strong>, distance and sometimes if necessary the altitude of the<br />

target can be determined from the measured antenna positi<strong>on</strong> and propagati<strong>on</strong> time of the pulsesignal.<br />

Weather <strong>radar</strong>s are pulse <strong>radar</strong>s.<br />

4.10. Doppler Radars<br />

C<strong>on</strong>venti<strong>on</strong>al <strong>radar</strong>s use MTI in order to remove clutter as explained above. This processing<br />

system is used almost entirely to eliminate unwanted clutter from the background, selecting as<br />

targets <strong>on</strong>ly those objects which move with some minimum velocity relative to the <strong>radar</strong> or to the<br />

fixed background. A more advanced type of system is the pulse Doppler <strong>radar</strong>, defined as a<br />

pulsed <strong>radar</strong> system which utilises the Doppler effect for obtaining informati<strong>on</strong> about the target,<br />

such as the target's velocity and amplitude, and not to use it for clutter rejecti<strong>on</strong> purposes <strong>on</strong>ly.<br />

In practice most pulsed Doppler <strong>radar</strong>s have evolved into forms which are quite distinct from the<br />

c<strong>on</strong>venti<strong>on</strong>al pulse <strong>radar</strong>s. Much higher PRF rates are used in order to eliminate or reduce the<br />

number of blind speeds. A blind speed exists when the PRF of the <strong>radar</strong> equals the Doppler shift<br />

frequency, therefore, the higher the PRF, the higher the first blind speed.<br />

A Pulse Doppler Radar is characterised by <strong>on</strong>e or more of the following:<br />

• A relative high PRF which results in ambiguous range and blind range problems.<br />

Unambiguous Doppler can be extracted up to the PRF, otherwise the Doppler<br />

frequencies<br />

are ambiguous.<br />

• A driven transmitter using a klystr<strong>on</strong> or travelling wave tube as a RF power amplifier is<br />

used rather than a magnetr<strong>on</strong> oscillator in order to obtain better frequency stability and<br />

hence phase stability. However, with the improvement of modern high-frequency<br />

magnetr<strong>on</strong>s some pulse Doppler <strong>radar</strong>s are using magnetr<strong>on</strong>s with suitable lock pulse<br />

arrangements.<br />

• A series of range gates or a movable range gate and a bank of clutter rejecti<strong>on</strong> filters<br />

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(Doppler filter bank to cover the Doppler spectrum) are used rather than a simple MTI<br />

system described above, in order to cancel clutter and to extract the Doppler frequency<br />

and amplitude comp<strong>on</strong>ents of the received signal.<br />

By extracting the Doppler characteristics of signals it is possible to achieve much better clutter<br />

cancellati<strong>on</strong> than in c<strong>on</strong>venti<strong>on</strong>al <strong>radar</strong>s, and the target’s radial velocity comp<strong>on</strong>ent can be<br />

calculated <strong>on</strong>ce the Doppler frequency is measured, in additi<strong>on</strong> it is possible by range gating to<br />

measure the Doppler and the amplitude of the returned signal in each <strong>radar</strong> cell. The locati<strong>on</strong> of<br />

the <strong>radar</strong> cell by measuring the return time, the positi<strong>on</strong> of the antenna (azimuth and elevati<strong>on</strong>) at<br />

the time the signal in the <strong>radar</strong> cell was received. All this processing is d<strong>on</strong>e digitally. A simple<br />

block shows the essential comp<strong>on</strong>ents of the Pulse Doppler Radar that is used for <strong>weather</strong><br />

observati<strong>on</strong>.<br />

4.11. Weather Radars<br />

Although these names refer to the applicati<strong>on</strong> of <strong>radar</strong>, there is a significant difference in the type<br />

of <strong>radar</strong> that is used which is worth to be illustrated. In general <strong>radar</strong>s measure the locati<strong>on</strong> of a<br />

target that is range, azimuth and height. The major distincti<strong>on</strong> between meteorological <strong>radar</strong> and<br />

other kinds of <strong>radar</strong>s lies in the nature of the targets. Meteorological targets are distributed in<br />

space and occupy a large fracti<strong>on</strong> of the spatial resoluti<strong>on</strong> cells observed by the <strong>radar</strong>. Weather<br />

<strong>radar</strong>s are pulsed <strong>radar</strong>s with Doppler capability. So we can call them as Pulsed Doppler Weather<br />

Radars. Weather <strong>radar</strong>s can operate in different frequency bands. So a classificati<strong>on</strong> can be made<br />

based <strong>on</strong> the frequency band as follows:<br />

L band <strong>radar</strong>s<br />

Those <strong>radar</strong>s operate <strong>on</strong> a wavelength of 15-30 cm and a frequency of 1-2 GHz. L band <strong>radar</strong>s<br />

are mostly used for clear air turbulence studies.<br />

S band <strong>radar</strong>s<br />

Those <strong>radar</strong>s operate <strong>on</strong> a wavelength of 8-15 cm and a frequency of 2-4 GHz. Because of the<br />

wavelength and frequency, S band <strong>radar</strong>s are not easily attenuated. This makes them useful for<br />

near and far range <strong>weather</strong> observati<strong>on</strong>. It requires a large antenna dish and a large motor to<br />

power it. It is not uncomm<strong>on</strong> for an S band dish to exceed 25 feet in size.<br />

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C band <strong>radar</strong>s<br />

Those <strong>radar</strong>s operate <strong>on</strong> a wavelength of 4-8 cm and a frequency of 4-8 GHz. Because of the<br />

wavelength and frequency, the dish size does not need to be very large. This makes C band<br />

<strong>radar</strong>s affordable for TV stati<strong>on</strong>s. The signal is more easily attenuated, so this type of <strong>radar</strong> is<br />

best used for short range <strong>weather</strong> observati<strong>on</strong>. Also, due to the small size of the <strong>radar</strong>, it can<br />

therefore be portable. The frequency allows C band <strong>radar</strong>s to create a smaller beam width using<br />

a smaller dish. C band <strong>radar</strong>s also do not require as much power as an S band <strong>radar</strong>.<br />

X band <strong>radar</strong>s<br />

Those <strong>radar</strong>s operate <strong>on</strong> a wavelength of 2.5-4 cm and a frequency of 8-12 GHz. Because of the<br />

smaller wavelength, the X band <strong>radar</strong> is more sensitive and can detect smaller particles. These<br />

<strong>radar</strong>s are used for studies <strong>on</strong> cloud development because they can detect the tiny water particles<br />

and also used to detect light precipitati<strong>on</strong> such as snow.. X band <strong>radar</strong>s also attenuate very easily,<br />

so they are used for <strong>on</strong>ly very short range <strong>weather</strong> observati<strong>on</strong>. Most major airplanes are<br />

equipped with an X band <strong>radar</strong> to pick up turbulence and other <strong>weather</strong> phenomen<strong>on</strong>. This band<br />

is also shared with some police speed <strong>radar</strong>s and some space <strong>radar</strong>s.<br />

K band <strong>radar</strong>s<br />

Those <strong>radar</strong>s operate <strong>on</strong> a wavelength of .75-1.2 cm or 1.7-2.5 cm and a corresp<strong>on</strong>ding<br />

frequency of 27-40 GHz and 12-18 GHz. This band is split down the middle due to a str<strong>on</strong>g<br />

absorpti<strong>on</strong> line in water vapour. This band is similar to the X band but is just more sensitive.<br />

This band also shares space with police <strong>radar</strong>s.<br />

4.12. Polarimetric Radars<br />

Polarimetric Radars are Doppler <strong>weather</strong> <strong>radar</strong>s with additi<strong>on</strong>al transmitting and processing<br />

functi<strong>on</strong>ality to allow to further compute additi<strong>on</strong>al informati<strong>on</strong> <strong>on</strong> the directi<strong>on</strong>ality of the<br />

reflected electromagnetic energy received.<br />

Most <strong>weather</strong> <strong>radar</strong>s, transmit and receive radio waves with a single, horiz<strong>on</strong>tal polarizati<strong>on</strong>.<br />

That is, the directi<strong>on</strong> of the electric field wave crest is aligned al<strong>on</strong>g the horiz<strong>on</strong>tal axis.<br />

Polarimetric <strong>radar</strong>s, <strong>on</strong> the other hand, transmit and receive both horiz<strong>on</strong>tal and vertical<br />

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polarizati<strong>on</strong>s. Although there are many different ways to mix the horiz<strong>on</strong>tal and vertical pulses<br />

together into a transmissi<strong>on</strong> scheme, the most comm<strong>on</strong> method is to alternate between horiz<strong>on</strong>tal<br />

and vertical polarizati<strong>on</strong>s with each successive pulse. That is, first horiz<strong>on</strong>tal, then vertical, then<br />

horiz<strong>on</strong>tal, then vertical, etc. And, of <str<strong>on</strong>g>course</str<strong>on</strong>g>, after each transmitted pulse there is a short listening<br />

period during which the <strong>radar</strong> receives and interprets reflected signals from the cloud.<br />

Since polarimetric <strong>radar</strong>s transmit and receive two polarizati<strong>on</strong>s of radio waves, they are<br />

sometimes referred to as dual-polarizati<strong>on</strong> <strong>radar</strong>s. The difference between n<strong>on</strong>-polarimetric and<br />

polarimetric <strong>radar</strong>s is illustrated below:<br />

4.13. Terminal Doppler Weather Radars (TDWR)<br />

Terminal Doppler Weather Radars a member of <strong>weather</strong> <strong>radar</strong>s family used generally at the<br />

airports for supporting the aviati<strong>on</strong> safety. TDWRs have the capability of detecting wind<br />

parameters indicating c<strong>on</strong>nective microbursts, gust fr<strong>on</strong>ts, and wind shifts. It provides a new<br />

capability for the disseminati<strong>on</strong> of <strong>radar</strong> derived, real-time, and warnings and advisories. The<br />

characteristics of the TDWR make it well suited for additi<strong>on</strong>al applicati<strong>on</strong>s. Its narrow beam and<br />

aggressive ground clutter suppressi<strong>on</strong> algorithms provide excellent data <strong>on</strong> boundary layer<br />

reflectivity and winds – in particular the locati<strong>on</strong>s of thunderstorm outflow boundaries.<br />

Similarly, its narrow beam (0.5 deg) could be useful for detecti<strong>on</strong> of severe <strong>weather</strong> signatures<br />

(e.g., tornado vortices) with small azimuth extent.<br />

4.14. Wind Profilers<br />

Wind profilers are specifically designed to measure vertical profiles of horiz<strong>on</strong>tal wind speed<br />

and directi<strong>on</strong> from near the surface to above the tropopause.<br />

Obtaining wind profiles c<strong>on</strong>sistently to the tropopause in nearly all <strong>weather</strong> c<strong>on</strong>diti<strong>on</strong>s requires<br />

the use of a relatively l<strong>on</strong>g wavelength <strong>radar</strong>. 404 MHz Wind profilers are relatively low-power,<br />

highly sensitive clear-air <strong>radar</strong>s, operating at a wavelength of 74 centimeters. The <strong>radar</strong>s detect<br />

fluctuati<strong>on</strong>s in the atmospheric density, caused by turbulent mixing of volumes of air with<br />

slightly different temperature and moisture c<strong>on</strong>tent. The resulting fluctuati<strong>on</strong>s of the index of<br />

refracti<strong>on</strong> are used as a tracer of the mean wind in the clear air. Although referred to as clear-air<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005 41


MODULE A- INTRODUCTION TO RADAR<br />

<strong>radar</strong>s, wind profilers are capable of operating in the presence of clouds and moderate<br />

precipitati<strong>on</strong>.<br />

At present, meteorological organizati<strong>on</strong>s use ballo<strong>on</strong> borne <strong>systems</strong> to measure profiles of wind,<br />

temperature and humidity from the ground to high up in the atmosphere. While current wind<br />

profiler <strong>radar</strong>s do not operati<strong>on</strong>ally measure all these parameters, they do have several<br />

advantages in comparis<strong>on</strong> to the ballo<strong>on</strong> based <strong>systems</strong>:<br />

# they can measure winds up to many kilometers from the ground (remote sensing)<br />

# they sample winds nearly c<strong>on</strong>tinuously<br />

# the winds are measured almost directly above the site<br />

# not <strong>on</strong>ly the horiz<strong>on</strong>tal but also the vertical air velocity can be measured<br />

# they have a high temporal and spatial resoluti<strong>on</strong><br />

# the cost per observati<strong>on</strong> is low<br />

42<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005


MODULE A- INTRODUCTION TO RADAR<br />

# they operate unattended in nearly all <strong>weather</strong> c<strong>on</strong>diti<strong>on</strong>s<br />

Since wind profiler <strong>radar</strong>s can be adapted to measure temperature profiles up to about 5 km<br />

when they are used in c<strong>on</strong>juncti<strong>on</strong> with a Radio-Acoustic Sounding System (RASS), the<br />

possibility to obtain temperatures profiles much more frequently than when using ballo<strong>on</strong><br />

tracking. No other measurement technique will present comparable advantages within the<br />

foreseeable future, including satellite borne sensors.<br />

4.15. Mobile <strong>radar</strong>s<br />

3-D mobile <strong>radar</strong> employs m<strong>on</strong>opulse technique for height estimati<strong>on</strong> and using electr<strong>on</strong>ic<br />

scanning for getting the desired <strong>radar</strong> coverage by managing the RF transmissi<strong>on</strong> energy in<br />

elevati<strong>on</strong> plane as per the operati<strong>on</strong>al requirements. It can be c<strong>on</strong>nected in air defence <strong>radar</strong><br />

network. The Radar is c<strong>on</strong>figured in three transport vehicles, viz., Antenna, Transmitter cabin,<br />

Receiver and Processor Cabin. The <strong>radar</strong> has an aut<strong>on</strong>omous display for stand-al<strong>on</strong>e operati<strong>on</strong>.<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005 43


MODULE A- INTRODUCTION TO RADAR<br />

5. REFERENCES:<br />

1. Radar for Meteorologist, R<strong>on</strong>ald E. Rinehart August 1997<br />

2. Solar Antenna Gain Measurement, R<strong>on</strong>ald E. Rinehart, Turkey, February 2004<br />

3. Radar Handbook, Merill I. Skolnik<br />

4. Doppler Radar and Weather Observati<strong>on</strong>s, Doviak R.J. & Zrnic D.S.<br />

5. Introducti<strong>on</strong> to Radar System, Merrill I. Skolnik<br />

6. Field and Wave Electromagnetics, David K. Cheng,1983<br />

7. Weather Radar Calibrati<strong>on</strong>, R. Jeffrey Keeler January, 2001<br />

8. Doppler Weather Radar System- Meteor 1000CUser Manuel and Documentati<strong>on</strong>-<br />

Gematr<strong>on</strong>ik GmbH<br />

12.July.2001<br />

9. RC-57A Weather Radar <strong>Training</strong> Document and User Manuel- Mitsubishi Electric<br />

Corp. 2002<br />

10. Radome Influence <strong>on</strong> Weather Radar Systems, Principle and Calibrati<strong>on</strong> Issues<br />

Gematr<strong>on</strong>ik GmbH Alexander Manz<br />

11. Principles of Radar- Wolfgang Manz 12.March .1999<br />

12. Radar Meteorology- Jürg Joss July.2004<br />

13. Technical Descripti<strong>on</strong> TDR Series-C Band Doppler Radar, Radtec Engineering<br />

14. Radar Range Folding and The Doppler Dilemma, Jeff Haby<br />

15. Doppler Radar, A detecting tool and measuring instrument in meteorology<br />

Current Science, Vol. 85, No. 3, 10 August 2003A.K. Bhatnagar, P. Rajesh Rao, S.<br />

Kalyanasundorom, S.B. Thampi, R. Suresh and J.P.Gupta<br />

16. Doppler Weather Radar System, Enterprise Electric Corp.<br />

17. Industrial Assessment of the Microwave Power Tube Industry, Department of<br />

Defense, U.S.A. April 1997<br />

18. Weather Watch Radar, BoM, Australia<br />

19. Radar Meteorology Doppler, Heikki Pohjoa, FMI<br />

20. Data Quality Improvements <strong>on</strong> AP Mitigati<strong>on</strong>, Range Velocity Mitigati<strong>on</strong>, Nati<strong>on</strong>al<br />

Weather Service, U.S.A<br />

21. Radar <strong>Training</strong> Informati<strong>on</strong>, NOAA<br />

44<br />

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MODULE A- INTRODUCTION TO RADAR<br />

22. Detecti<strong>on</strong> of ZDR abnormalities <strong>on</strong> operati<strong>on</strong>al polarimetric <strong>radar</strong> in Turkish<br />

<strong>weather</strong> <strong>radar</strong> network, WMO- TECO 2005, TSMS, Oguzhan Sireci, 4th.May.2005<br />

23. Modernizati<strong>on</strong> of Observati<strong>on</strong> Network in Turkey, TECO 2005, TSMS, Ercan<br />

Buyukbas, 4th.May.2005<br />

24. Radar Basics, Renato Croci<br />

25. Feasibility Report for Turkey Radar Network, BoM, Australia,2000<br />

26. Weather Radar Principles, Firat Bestepe, TSMS, 2005<br />

27. Principles of Meteorological Doppler Radar, Distance Learning Operati<strong>on</strong>s Course,<br />

Instructi<strong>on</strong>al Comp<strong>on</strong>ent 5.3. Ver: 0307<br />

28. Notes <strong>on</strong> Radar Basics, Serkan Eminoglu, TSMS,2004<br />

29. Radar Basics, Radar <strong>Training</strong> Informati<strong>on</strong>,NOAA<br />

30. Turkish Radar Network, Hardware Maintenance of Weather Radars, <strong>Training</strong><br />

Notes, Ercan Büyükbas, Oguzhan Sireci, Aytac Hazer, Ismail Temir, Cihan Gozubuyuk,<br />

Abdurrahman Macit, M.Kemal Aydin, Mustafa Kocaman, 2002<br />

31. Weather Radar Maintenance Procedures and Measurements, TSMS, Aytac Hazer,<br />

Cihan Gozubuyuk, 2005<br />

32. Operati<strong>on</strong>al Use of Radar for Precipitati<strong>on</strong> Measurements in Switzerland<br />

Jürg Joss(1)Bruno Schädler(2) Gianmario Galli(1) Remo Cavalli(1) Marco Boscacci(1)<br />

Edi Held(1) Guido Della runa(1) Giovanni Kappenberger(1) Vladislav Nespor(3) Roman<br />

Spiess(3) Locarno, 23.Sep.1997<br />

33. Radar Lecture Notes and Articles available in internet<br />

34. Booklets, reports and guidelines published by WMO<br />

35. Technical Brochures of Radar Manufacturers<br />

TURKEY RADAR TRAINING 1.0 / ALANYA 2005 45

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