Bibcode
Asensio Ramos, A.; Collados, M.
Bibliographical reference
Applied Optics IP, vol. 47, Issue 14, pp.2541-2549
Advertised on:
5
2008
Citations
6
Refereed citations
5
Description
The polarization analysis of light is typically carried out using
modulation schemes. The light of an unknown polarization state is passed
through a set of known modulation optics, and a detector is used to
measure the total intensity passing the system. The modulation optics is
modified several times, and, with the aid of several such measurements,
the unknown polarization state of the light can be inferred. How to find
the optimal demodulation process has been investigated in the past.
However, since the modulation matrix has to be measured for a given
instrument and the optical elements can present problems of
repeatability, some uncertainty is present in the elements of the
modulation matrix or covariances between these elements. We analyze in
detail this issue, presenting analytical formulas for calculating the
covariance matrix produced by the propagation of such uncertainties on
the demodulation matrix, on the inferred Stokes parameters, and on the
efficiency of the modulation process. We demonstrate that even if the
covariance matrix of the modulation matrix is diagonal, the covariance
matrix of the demodulation matrix is in general nondiagonal because
matrix inversion is a nonlinear operation. This propagates through the
demodulation process and induces correlations on the inferred Stokes
parameters.
Related projects
Solar and Stellar Magnetism
Magnetic fields are at the base of star formation and stellar structure and evolution. When stars are born, magnetic fields brake the rotation during the collapse of the mollecular cloud. In the end of the life of a star, magnetic fields can play a key role in the form of the strong winds that lead to the last stages of stellar evolution. During
Tobías
Felipe García
Magnetism, Polarization and Radiative Transfer in Astrophysics
Magnetic fields pervade all astrophysical plasmas and govern most of the variability in the Universe at intermediate time scales. They are present in stars across the whole Hertzsprung-Russell diagram, in galaxies, and even perhaps in the intergalactic medium. Polarized light provides the most reliable source of information at our disposal for the
Tanausú del
Pino Alemán