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Fields from a Fractal Antennae

A current pulse propagates with speed along a fractal structure. At the n line element with orientation and length , which is parametrized by , the current is given by where is the path length along the fractal (or if you prefer a phase shift). The radiation field is the superposition, with the respective phases, of the small line current elements that form the fractal. For a set of line elements, such as shown in the example diagram of Fig. 25, the Hertz vector is given by

 

where is the vector from the beginning of the line element to the field position , is the frequency and .

  
Figure 25: A diagram that explains all the variables and coefficients

We must realize that in general Eq. 10 for is very complicated, but we are interested in the far field of the small line elements (). Therefore, we can take the far field approximation of the small line elements to obtain a closed form solution for the Fourier transformed fields as

where the geometric factor is given by

Note that even though we are in the far field of the small line elements, we can be in fact in the intermediate field with respect to the global fractal structure. Therefore, phase correlations over the fractal can be extremely relevant, and produce spatially nonuniform radiation fields. We then invert the Fourier transform of the field to real time and obtain the spatio-temporal radiation pattern due to the fractal discharge structure

 

where

can be calculated exactly for the current described above, and where

The value of and correspond to the causal time delays from the two end points of the line element.

Before finishing this section we want to mention that there is an inherent symmetry in the radiation fields. In general we will assume that the current is given by where is the step function, and . Note that the total charge discharged by this current is Q= where is the decay time of the current. But since the current propagates along the fractal, the radiation fields at a given position in space will last for a time given by where s is the largest path length along the fractal. The fields are invariant as long as , and are kept constant in the transformation. Such scaling can become relevant in studying the properties of radiation fields from fractal antennae.

In general we will use the power density where 1/ is the impedance of free space, as a natural description for the amount of power radiated through a cross-sectional area.



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Next: The Far field Up: No Title Previous: Fields from a