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ELECTROMAGNETICS AND APPLICATIONS Lecture 22 Aperture Antennas Diffraction Luca Daniel.

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Presentation on theme: "ELECTROMAGNETICS AND APPLICATIONS Lecture 22 Aperture Antennas Diffraction Luca Daniel."— Presentation transcript:

1 ELECTROMAGNETICS AND APPLICATIONS Lecture 22 Aperture Antennas Diffraction Luca Daniel

2 L21-2 Review of Fundamental Electromagnetic Laws Electromagnetic Waves in Media and Interfaces Digital & Analog Communications Wireless Communications oRadiation Fundamentals oTransmitting Antennas, Gain oReceiving Antennas; Effective Area oAperture Antennas; Diffraction  Examples of aperture antennas  Far field radiation from aperture antenna  Connection with Fourier Transform  Ex. rectangular aperture antenna  Gain and effective area of an aperture antenna  Slit diffraction Acoustic waves and Acoustic antennas e.g. speakers, musical instruments, voice Outline Today

3 Course Outline and Motivations Electromagnetics: –How to analyze and design antennas Applications –wire antennas (e.g. inside your iPhone, or wireless router) –aperture antennas (e.g. satellite, radar, parabola)

4 Aperture Antennas Dense phased arrays If each element is cancelled by another a distance D/2 away, the total is a null. => First null at  ≈ /D Aperture antennas: Derivation of far-field aperture radiation: Parabolic reflector Aperture screen Phased array /2  null cancel D 12- element array 1) Find equivalent current J s that would produce the same field in the aperture 2) Find the far fields radiated by each infinitesimal element of J s 3) Add up the contributions from all equivalent currents in the aperture 4) Simplify the expressions by using small-angle approximations => Fourier relationship between aperture and far fields ≈ apertures D 

5 Far-Field Radiation from Aperture Antennas Equivalent surface current Corresponding radiated far-field: JsJs z y x z y  aperture A r qp q p JsJs top view p k from Magnetic field boundary conditions: k

6 Far Field is the Fourier Transform of Aperture Field Radiated far field: Fourier relationship: ( time  frequency) Fraunhofer approximation (else, Fresnel) Fourier relationship: (space  k angle) z x q rqrq roro r qp x z y aperture A xx yy q p sin   1 xx roro side view p r qp p p F F 

7 Example: Rectangular Aperture For a distant observer close to the z axis: LxLx x’ ≈  x d d xx Null≈( /L x )d The Fourier transform of a box is a sinc Area rule: Area in angle domain

8 Aperture Antenna Gain and Effective Area Rectangular Aperture: G(  x,  y ) = I(  x,  y ) / (P t /4  r 2 ) where I(  x,  z ) = |E ff | 2 /2  o P t = L x L y |E o | 2 /2  o G(  x,  z ) = L x L y (4  / 2 )sinc 2 (  x L x / )sinc 2 (  y L y / ) G max = A (4  / 2 ) where A = L x L y [note: sin(    1 as   0] Hence, in theory A e =A i.e. for an aperture the effective area is the geometrical area But in practice, A e  0.65 A (i.e. “aperture efficiency”  65% x z y LxLx LyLy aperture xx yy xx yy Null at  y = /L y Null at  x = /L x First sidelobe G(  x,  y ) |E ff | 2 =|E o | 2 /( r) 2 ( L x L y ) 2 sinc 2 (  x L x / )sinc 2 (  y L y / )

9 Example: Slit Diffraction Pair of rectangular slots: Uniform illumination * = Fourier transform Spatial domain D L = Angular domain /D 0 /L x Convolution Multiplication  (x,z-D/2) z=-D/2 D z z=+D/2


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