Polarization Calibration: Difference between revisions

From EOVSA Wiki
Jump to navigation Jump to search
Line 11: Line 11:
One problem is that there is generally a non-zero delay in Y with respect to X.  This creates phase slopes in XY* and YX* from which we can determine the delay very accurately.  As a check,
One problem is that there is generally a non-zero delay in Y with respect to X.  This creates phase slopes in XY* and YX* from which we can determine the delay very accurately.  As a check,


:<math> Stokes I = \frac{RR^* + LL^*}{2} = XX^* + YY^*</math>
:<math> Stokes \, I = \frac{RR^* + LL^*}{2} = XX^* + YY^*</math>


:<math> Stokes V = \frac{RR^* - LL^*}{2} = i(XX^* - YY^*)</math>
:<math> Stokes \, V = \frac{RR^* - LL^*}{2} = i(XX^* - YY^*)</math>


For completeness:
For completeness:


:<math> Stokes \, Q = XX^* - YY^* </math>
:<math> Stokes \, Q = XX^* - YY^* \\


:<math> Stokes U = XY^* - YX^* </math>
        Stokes \, U = XY^* - YX^* </math>


:<math> P_{linear} = \sqrt{U^2 + Q^2} </math>
:<math> P_{linear} = \sqrt{U^2 + Q^2} </math>

Revision as of 20:10, 24 September 2016

Linear to Circular Conversion

At EOVSA’s linear feeds, in the electric field the linear polarization, X and Y, relates to RCP and LCP (R and L) as:

In terms of autocorrelation powers, we have the 4 polarization products XX*, YY*, XY* and YX*, where the * denotes complex conjugation. The quantities RR* and LL* are then

One problem is that there is generally a non-zero delay in Y with respect to X. This creates phase slopes in XY* and YX* from which we can determine the delay very accurately. As a check,

For completeness:

Failed to parse (syntax error): {\displaystyle Stokes \, Q = XX^* - YY^* \\ Stokes \, U = XY^* - YX^* }

Polarization Mixing Correction

Due to relative feed rotation between az-al mounted antennas and equatorial mounted antennas