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For the moment, it will be assumed that there is a single point source
at an arbitrary position (direction)
=
(
,
)
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'
, which is
related to the so-called `Stokes vector'
(
,
)
of the observed source by a matrix equation,
The subscripts
and
are the labels of the two feeds that make up the interferometer. The subscripts
and
are the labels of the two output IF-channels from each
feed.1
The `Stokes matrix'
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'
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
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[2]
[3]. Using equation 1:
Mueller matrices are useful in simulation, when studying the effect
of instrumental effects on a test source
(
,
).
They can be easily generalised to the full M.E. (see section
3).