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The coverage
Using a Cartesian coordinate system
with towards the pole, towards the meridian, and towards East, the
conversion matrix to is
|
(2.46) |
where
are the hour angle and declination of the phase tracking
center.
Eliminating from Eq.2.46 gives the equation of an ellipse:
|
(2.47) |
The coverage is an ensemble of such ellipses. The choice of antenna
configurations is made to cover the plane as much as possible.
Baseline measurement
Assume there is a small baseline error,
(
). The phase error is
Hence, if we observe sources, we have for each source
|
(2.50) |
i.e. a linear system in (
), with equations
and 4 unknown (including the arbitrary phase ). This can be used
to determine the baselines from phases measured on a set of sources with
known positions
.
From the shape of Eq.2.49, one can see that the
determination of
requires large variations in
, preferably at declination
, while that of
requires large variations in . However,
in Eq.2.50 is multi-valued (the
ambiguity...). Retaining the function in the [] interval
only, the system to solve is in fact
|
(2.51) |
which is a linear system of equations only if
are
small enough so that the shifted modulo function is the identity. Baseline
determination usually proceeds through a ``brute force'' technique, by making a grid
search (with phase steps) around the most likely values for .
Next: 3. Millimetre Very Long
Up: 2. Millimetre Interferometers
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Anne Dutrey