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Principles of Modern Radar - Volume 2 1891121537

Principles of Modern Radar - Volume 2 1891121537

Principles of Modern Radar - Volume 2 1891121537

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218 CHAPTER 6 Spotlight Synthetic Aperture <strong>Radar</strong>specific main lobe and sidelobe behavior. Interesting features <strong>of</strong> numerous such windowingfunctions are described by Harris [12].When we let B grow to be arbitrarily large, the rect function becomes infinitelywide and the corresponding sinc funtion grows infinitesimally narrow. Without rigorousjustification <strong>of</strong> the assertion, we simply state the following transform pair:1 ⇔ δ(t) (6.11)where δ(t) is the well-known Dirac delta function that takes the value 1 at t = 0 and zeroeverywhere else [9]. For our purposes, the important feature <strong>of</strong> the delta function is thatequations (6.3) and (6.11) can be combined to find that its Fourier transform is a complexsinusoid:e − jωt 0⇔ δ(t − t 0 ) (6.12)This property holds in higher dimensions, and it is critical to understanding many aspects<strong>of</strong> SAR imaging. Each point in a scene can be idealized as a shifted and weighted deltafunction where the weight corresponds to the reflectivity at the location implied by theshift.6.2.3 Spatial Frequency and Plane WavesThe familiar symbols t and ω are used to represent time and temporal frequency, respectively.Equally useful is the notion <strong>of</strong> spatial frequency, symbolized as k with units <strong>of</strong>radians per meter. While temporal frequency ω represents the number <strong>of</strong> radians a wavecycles through per unit time, the spatial frequency represents the number <strong>of</strong> radians aharmonic (or single frequency) wave passes through per unit length. The wavenumber is<strong>of</strong>ten written as k = 2π/λ, or equivalently k = ω/c since c = λf . The wavenumbervector k = [k x k y k z ] T is used to describe the spatial frequency in multiple dimensions.The Fourier transform <strong>of</strong> a shifted delta function, given in equation (6.12), also holdsin higher dimensions:δ(x − x 0 ) ⇔ exp{− jk · x 0 } (6.13)The two-dimensional case is obtained when x 0 has no z component. These two- and threedimensionalcomplex sinusoids are called plane waves because contours <strong>of</strong> constant phaseare parallel. Some examples are shown in the right-hand column <strong>of</strong> Figure 6-2. Given thata delta function in one domain transforms into a plane wave in the other, the frequency <strong>of</strong>this plane wave is proportional to the impulse’s distance from the origin. The orientation<strong>of</strong> the plane wave corresponds to the location <strong>of</strong> the delta function around the origin. Inthis fashion each point in the SAR image corresponds to a unique spatial frequency, ortwo-dimensional complex sinusoid in the Fourier domain.The SAR image is just like any other signal in that it is composed <strong>of</strong> (and can beexpressed as) the weighted sum <strong>of</strong> sinusoids. SAR practitioners rely heavily on thisFourier-oriented mindset. The relevance to SAR is that we can infer δ(x − x 0 ) by makingmeasurements in the frequency domain and then Fourier transforming the result toobtain the image. The amplitude and location <strong>of</strong> the delta function will be shown to correspondto the amplitude <strong>of</strong> the scene reflectivity at a particular location on the ground.Since the imaging process is linear, superposition holds and we are able to reconstruct the

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