illum_parabolic¶
- pyoof.aperture.illum_parabolic(x, y, I_coeff, pr)[source]¶
Illumination function, \(E_\mathrm{a}(x, y)\), parabolic taper on a pedestal, sometimes called apodization, taper or window. Represents the distribution of light in the primary reflector. The illumination reduces the side lobe effect in the FT and it is a (feed) receiver property.
- Parameters
- x
Quantity
Grid value for the \(x\) variable in length units.
- y
Quantity
Grid value for the \(y\) variable in length units.
- I_coeff
list
List which contains 5 parameters, the illumination amplitude, \(A_{E_\mathrm{a}}\), the illumination taper, \(c_\mathrm{dB}\) and the two coordinate offset, \((x_0, y_0)\). The illumination coefficients must be listed as follows,
I_coeff = [i_amp, c_dB, q, x0, y0]
, with units as dimensionless, decibels and length, respectively. The coefficientq
varies between 1 and 2 for reflector antennas.- pr
astropy.units.quantity.Quantity
Primary reflector radius in length units.
- x
- Returns
- Ea
ndarray
Illumination function, \(E_\mathrm{a}(x, y)\).
- Ea
Notes
The parabolic taper on a pedestal has the following mathematical formula,
\[E_{\mathrm{a}} (\rho') = C + (1 - C) \cdot \left[ 1 - \left( \frac{\rho'}{R} \right)^2 \right]^q,\]\[C=10^{\frac{c_\mathrm{dB}}{20}}.\]