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The very great effort going into giving the ALMA very high sensitivity
for mapping of total intensity also will yield high sensitivity for
polarization work so long as that sensitivity is not compromised by the
instrumental design. The fact that the ALMA will have dual receivers
with feeds sensitive to orthogonal polarizations is the first necessary
step. But if that system is to achieve its potential for polarization
work, the design must have a focus on the effect on polarization of all
aspects of the system.
Polarization is usually less than 5%, and over large spatial areas the
percentage polarization is 1% or less. Hence, the dynamic range that can
be achieved is automatically significantly lower than for intensity
observations. In order not to further reduce sensitivity, one would like
to be able to map polarization to the limits set by thermal noise rather
than instrumental polarization.
Al Wootten
2000-04-04