Ruze's equation

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Ruze's equation is an equation relating the gain of an antenna to the RMS of the random surface errors. The equation is applicable to parabolic reflector and antennas, and recently extended to phased arrays. The equation is named after John Ruze who introduced the equation in a paper he wrote in 1952. The equation states that the antenna's gain is inversely proportional to the exponential of the square of the RMS surface errors. Mathematically, the equation for parabolic reflector antennas can be expressed as:

${\displaystyle G\left(\epsilon \right)=G_{0}\,\,e^{-\left({\frac {4\pi \epsilon }{\lambda }}\right)^{2}}}$

where ${\displaystyle \displaystyle \epsilon }$ is the surface RMS errors of the reflector, ${\displaystyle \displaystyle \lambda }$ is the wavelength, and ${\displaystyle \displaystyle G_{0}}$ is the gain of the antenna in the absence of surface errors.

The equation is often expressed in decibels as:

${\displaystyle G\left(\epsilon \right)=g_{0}\,-\,685.81\left({\frac {\epsilon }{\lambda }}\right)^{2}}$ (dB)

where ${\displaystyle -685.81=10\log _{10}\left(e^{{-\left(4\pi \right)}^{2}}\right)}$ and ${\displaystyle g_{0}=10\log _{10}G_{0}}$

Video Ruze's equation

Application to phased array

Ruze's equation, which was originally derived for parabolic reflectors has been extended to phased array applications. For phased arrays, the equation is slightly modified, differing by a factor of 2 in the exponential, to give

${\displaystyle G\left(\epsilon \right)=G_{0}\,\,e^{-\left({\frac {2\pi \epsilon }{\lambda }}\right)^{2}}}$

The factor of 2 difference between the equation for the phased array and the equation for reflectors is that the electromagnetic wave goes in only one direction for phased arrays, but it goes back and forth in reflectors (the wave is reflected).

Consequently, when expressed in dB, Ruze's equation for phased arrays has a different coefficient, namely:

${\displaystyle G\left(\epsilon \right)=G_{0}\,-\,171.45\left({\frac {\epsilon }{\lambda }}\right)^{2}}$ (dB)

where ${\displaystyle \displaystyle \epsilon }$ is the RMS of the z-directed positional errors of the array elements, and as before, ${\displaystyle \displaystyle \lambda }$ is the wavelength.

Maps Ruze's equation

References

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Further reading

• The Radio Astronomy tutorial presented by MIT's Haystack Observatory (Section 6.2.3)

Source of the article : Wikipedia