Post-Processing Results in POSTFEKO
After solving the Three_Spheres_VPol_MoM.cfx model, the post-processing is done in POSTFEKO using the PF_ISAR.lua macro.

- Far field request
- Select the RCS far field request to process.
- Windowing function
-
Hamming
Dirichlet
Bartlett
Blackman
- Interpolate to Cartesian grid
- The 2D FFT requires that the X and Y distances should be uniformly spaced.
The basic ISAR implementation assumes that the angle range is small enough
such that the polar sampling approximates a Cartesian grid. The small angle
range assumption can be relaxed by transforming the polar grid to Cartesian.
This reduces smearing and shift of the scattering points and increasing
accuracy of the resulting ISAR image.
Figure 1. Polar to Cartesian transformation. - Component
- Specify which E-field component to use to generate the ISAR result.
Supported options are:
- Theta
- Phi
- LHC (Left Hand Circular)
- RHC (Right Hand Circular)
- Image offset
- Offset distance of the ISAR image above the plane wave workplane.
- Resample factor
- Factor used to up sample the image resolution to create a smoother image with more points. Note it does not change the underlying image resolution based on the frequency and angular information.
- Create 3D view
- Generates a normal view of the partially transparent ISAR image with RCS data displayed in dB.
- Find local maxima
- Calculates the specified number of local maxima in descending order in the ISAR image.
- Export local maxima to CSV
- Export the specified number of local maxima to a CSV file. Find local maxima has to be checked for this to work.
- Number of local maxima
- The number of local maxima to find.

Figure 2. The Angle selection dialog for specifying the viewing angle.

Figure 3. The Angle selection dialog for specifying the angular range.
The ISAR images associated with the XY_plane and UV_plane solution configurations are shown below. For this example, a resampling factor of 2 was used with default values for the rest of the input parameters.

Figure 4. ISAR image (3.5 m x 3 m) obtained from the XY_plane solution configuration (left) and the UV_plane solution configuration (right).

Figure 5. RCS versus X position for the Y coordinates of points A1, A2 and A3.