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Relations exist between the brightness temperatures of passive remote sensing and the bistatic coefficients of active remote sensing when the medium is of uniform temperature. The expressions were derived in Volume I, 3, Section 5. In this section, we derive a similar expression for nonuniform temperature distribution. An expression will be derived relating the thermal radiated field intensity of a medium with nonuniform temperature distribution to the electromagnetic fields in the problem of active remote sensing. Specifically, it is shown that the thermal radiated field intensity is equal to a constant times the integration of the product of the temperature distribution and the divergence of the Poynting's vector for the problem of active remote sensing. The derivation is based on the field equations of a medium of discrete scatterers and the fluctuation-dissipation theorem. The key quantity to utilize in the derivation is the dyadic Green's function of the random medium, which is common to both problems and is also reciprocal. In the following, active and passive remote sensing problems will be labeled as Problems A and B, respectively.

One of the most useful Silverlight controls in adding a professional look to applications is the Image control. The Image control allows you to add images to your applications as a codemanageable control by simply referencing their URI in the Source property.

Problem A:

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In Section 3 we have seen the importance of the pair distribution function in calculating the lowest-order scattered intensity because the field and field conjugates originate from different scatterers. In some problems the scatterers occur in clusters. For example, in a vegetation canopy the branches and leaves can occur in clusters, so that they are locally densely distributed and not uniformly dense. In such a case the pair distribution function depends on whether the two scatterers arc in the same cluster or in different clusters. In 7 of Volume II, we have performed Monte Carlo simulations for collections of clusters of scatterers. In the following, we consider the scattering of a layer of thickness D of point scatterers when the scatterers can be in clusters. We assume that the particles may occur in clusters with N s particles in each cluster. Note that N., may not be a large number. For the case of nonclustering, N s = 1. The number of clusters in the layer is N c with N Nc = (3.6.1a) Ns and N, N c - t 00. The center of each cluster is at 'fa, Q = 1,2, ... , N c (Fig. 3.6.1). The N s scatterers in each cluster Q are labeled as secondary scatterers, with indices ja, ja = 1, ... , N s . The location of the ja scatterer is at

(3.6.1b)

The Height and Width properties allow you to set the size of the Image control and the Stretch property defines how the image file fills that space. As shown in the following code, the Stretch property can be set to None (default), Fill, Uniform, and UniformToFill:

with ja = 1, ... N s . The volume occupied by the clusters is Ve, where Vc does not have to be large compared with wavelength. Thus the single-particle

z=()

...... tt", :.

<Image Source= image2.jpg Height= 100 Width= 100 Margin= 10,0,0,0 HorizontalAlignment= Left /> <Image Source= image2.jpg Stretch= Fill Height= 100 Width= 100 Margin= 120,0,0,0 HorizontalAlignment= Left /> <Image Source= image2.jpg Stretch= Uniform Height= 100 Width= 100 Margin= 230,0,0,0 HorizontalAlignment= Left /> <Image Source= image2.jpg Stretch= UniformToFill Height= 100 Width= 100 Margin= 340,0,0,0 HorizontalAlignment= Left />

...... ..... :.

..... :.

'. t,: t,' "::

Figure 3.6 shows the rendered Image controls from the previous code. Even though it is the same image, the Stretch property changes how the image actually is rendered. None and Uniform settings simply display the image uniformly in the space provided by the Height and Width settings. Fill stretches the image to fill the space. UniformToFill keeps the image uniform but clips it so that it fills the entire space specified by Height and Width.

. .'

(3.6.2) (3.6.3)

For the sake of simplicity, we have a.'isumed that the primary cluster location and the secondary scatterer locations are independent. In taking averaging, we note that N, N c and V -----; 00, while N., and Vc , the number of particles in each cluster and the volume occupied by each cluster are finite. The layer D is such that A, l D lmf]J' The cluster size Vc is related also to I and the layer thickness D must contain many clusters so that D Furthermore, we let

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