Far Field Patterns of Aperture Antennas
   
   
       Joachim Köppen DF3GJ ... Kiel, Aug 2016
   
  
  
Some brief explanations
    
      - This tool computes the antenna pattern of square and circular dishes,
          illuminated either uniformly or with a few laws. This is done for 
          a point source, which gives the theoretical pattern.
          One enters the relevant data and clicks the point source
          button. The result is shown as a blue curve. The magenta markings indicate
          the HPBW, and the green curve shows the width of the equivalent lobe with 
          solid angle ΩA if all the power emitted by the antenna (in the 
          displayed range) were radiated at constant strength.
 
      - The computation of non-uniform illumination patterns takes some time!
 
      - The pattern can also be computed for a few types of extended sources 
          which are specified by their angular diameter. If a point source pattern
          is displayed, one clicks the extended source button, and the result
          is shown as a red curve. The gray curve indicates the brightness across the 
          face of the source.
 
      - Note that the 1 D source patterns give only approximate results, they require
          less time, so they can be good for a first rough view!
 
      - From the observed pattern the FWHM (i.e. apparent HPBW), solid angle ΩA,
          and the beam filling factor of the source are given.
 
      - Display: one may set the maximum offset angle and choose between
          linear, logarithmic and deciBel ordinates.
 
      - overplot permits to superpose different plots, in order to compare 
          different patterns.
 
      - The mouse position gives the coordinates of that point, allowing to read
          numerical values from the plot. In some browsers, these values may not 
          correspond to the plot. If this happens, keep this page in its initial
          top-left corner position.
 
      - Please note that due to the finite accuracy chosen to get reasonably
          fast computations, one may get weird results if one pushes the tool
          to extreme choices of parameters! For example, a source diameter larger
          than 10 times the antenna's HPBW  - which nobody really needs to compute -
          leads to perturbations in the central part of the pattern ...