Polarization Ellipse: Understanding 2*Psi Angle

AI Thread Summary
In radio astronomy, the orientation angle of a polarization ellipse is represented by tan(2 * Psi) = S2/S1, where S2 and S1 are Stokes parameters. The factor of 2 in the angle accounts for the periodic nature of polarization, as rotating the polarization vector by 180 degrees describes the same ellipse, making the functions periodic over 180 degrees instead of 360 degrees. This relationship allows for consistent results when polarizers are rotated by 90 degrees. Understanding this concept is crucial for accurate interpretation of polarization data in radio astronomy. The discussion highlights the mathematical foundation behind the use of the 2 * Psi angle in describing polarization ellipses.
Steleo
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Hello all

In radio astronomy the orientation angle of an ellipse is usually quoted as
tan(2 *Psi) = S2/S1

Where S2 and S1 are the stokes parameters.

Does anyone know or can point me to a reference as to why the 2 * psi should be in there? The angle of the axis in the ellipse should be able to go between -Pi/2 to Pi/2? Does it have something to do with the fact that you can rotate all your polarisers by 90 degrees and get the same result?

Cheers
 
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http://en.wikipedia.org/wiki/Stokes_parameters

If you take the polarization vector and rotate it 180 degrees, you are describing the same ellipse. That's where the factor of 2 comes from, to make those functions periodic over 180 degrees instead of 360 degrees. Not sure if that's exactly what you were talking about when you said rotate both of your polarizers 90 deg., but it's the same idea.
 
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