Polarization Calibration: Difference between revisions
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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> Stokes \, Q = XX^* - YY^* \\ | ||
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