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Next: The feed-based instrumental Jones matrices Up: The MEASUREMENT EQUATION of a generic radio telescope Previous: INTRODUCTION


THE M.E. FOR A SINGLE POINT SOURCE

For the moment, it will be assumed that there is a single point source at an arbitrary position (direction) $ \vec{{\rho}}\,$ = $ \vec{{\rho}}\,$($ \sf l$,$ \sf m$) w.r.t. the fringe-tracking centre, and that observing bandwidth and integration time are negligible. Multiple and extended sources, and the effects of non-zero bandwidth and integration time will be treated for the Full Measurement Equation in section 3.

For a given interferometer, the measured visibilities can be written as a 4-element `coherency vector' $ \vec{{V}}_{{{{\sf i}{\sf j}}}}^{{}}$, which is related to the so-called `Stokes vector' $ \vec{{I}}\,$($ \sf l$,$ \sf m$) of the observed source by a matrix equation,

$\displaystyle \vec{{V}}_{{{{\sf i}{\sf j}}}}^{{}}$  = $\displaystyle \left(\vphantom{\begin{array}{c}
{\sf v}_{{\sf i}{\sf p}\,{\sf j...
...f j}{\sf p}}\\
{\sf v}_{{\sf i}{\sf q}\,{\sf j}{\sf q}}
\end{array}}\right.$$\displaystyle \begin{array}{c}
{\sf v}_{{\sf i}{\sf p}\,{\sf j}{\sf p}}\\
{...
... q}\,{\sf j}{\sf p}}\\
{\sf v}_{{\sf i}{\sf q}\,{\sf j}{\sf q}}
\end{array}$$\displaystyle \left.\vphantom{\begin{array}{c}
{\sf v}_{{\sf i}{\sf p}\,{\sf j...
...f j}{\sf p}}\\
{\sf v}_{{\sf i}{\sf q}\,{\sf j}{\sf q}}
\end{array}}\right)$  = ($\displaystyle \sf J_{{{\sf i}}}^{}$ $\displaystyle \otimes$ $\displaystyle \sf J_{{{\sf j}}}^{{\ast}}_{{}}$$\displaystyle \sf S$ $\displaystyle \left(\vphantom{\begin{array}{c}
I\\  Q\\  U\\  V
\end{array}}\right.$$\displaystyle \begin{array}{c}
I\\  Q\\  U\\  V
\end{array}$$\displaystyle \left.\vphantom{\begin{array}{c}
I\\  Q\\  U\\  V
\end{array}}\right)_{{{\sf l},{\sf m}}}^{}$ (1)

The subscripts $ \sf i$ and $ \sf j$ are the labels of the two feeds that make up the interferometer. The subscripts $ \sf p$ and $ \sf q$ are the labels of the two output IF-channels from each feed.1

The `Stokes matrix' $ \sf S$ is a constant 4 x 4 coordinate transformation matrix. It is discussed in detail in section 4 below. The real heart of the M.E. is the `direct matrix product' $ \sf J_{{{\sf i}}}^{}$ $ \otimes$ $ \sf J_{{{\sf j}}}^{{\ast}}_{{}}$ of two 2 x 2 feed-based Jones matrices.

The `Stokes-to-Stokes' transmission of a Stokes vector through an `optical' element may be described by multiplication with a 4 x 4 Mueller matrix $ \cal {M}$$\scriptstyle \sf i$$\scriptstyle \sf j$ [2] [3]. Using equation 1:

$\displaystyle \vec{{I}}^{{{out}}}_{{}}$($\displaystyle \sf l$,$\displaystyle \sf m$)  = $\displaystyle \sf S^{{-1}}_{}$ $\displaystyle \vec{{V}}_{{{{\sf i}{\sf j}}}}^{{}}$  = $\displaystyle \sf S^{{-1}}_{}$ ($\displaystyle \sf J_{{{\sf i}}}^{}$ $\displaystyle \otimes$ $\displaystyle \sf J_{{{\sf j}}}^{{\ast}}_{{}}$$\displaystyle \sf S$ $\displaystyle \vec{{I}}^{{{in}}}_{{}}$($\displaystyle \sf l$,$\displaystyle \sf m$)  = $\displaystyle \cal {M}$$\scriptstyle \sf i$$\scriptstyle \sf j$($\displaystyle \sf l$,$\displaystyle \sf m$$\displaystyle \vec{{I}}^{{{in}}}_{{}}$($\displaystyle \sf l$,$\displaystyle \sf m$) (2)

Mueller matrices are useful in simulation, when studying the effect of instrumental effects on a test source $ \vec{{I}}\,$($ \sf l$,$ \sf m$). They can be easily generalised to the full M.E. (see section 3).



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