[fitswcs] Polarization codes
Paddy Leahy
j.p.leahy at manchester.ac.uk
Tue Mar 11 14:26:15 EDT 2008
Dear All,
I was surprised to find recently that the current FITS WCS
conventions do not appear to provide an unambiguous (i.e. machine-
interpretable) way of specifying such routine polarization products as
polarization angle and fractional polarization. I'm not sure if this
mailing list is the right place to raise the issue but since the current
"Stokes" codes were defined in WCS paper I it seems a good place to start.
Reminder: on the current definition (WCS Paper I, Table 7), the official
stokes parameters I, Q, U, V are assigned STOKES 1,2,3,4, while various
products such as RR through XY (which are linear combinations of I,Q,U,V)
are assigned STOKES -8 through -1.
I propose that we extend the existing list to include all the meaningful
non-linear combinations of I,Q,U,V. I may be naive, but it seems to me
that there are only a small number of such non-linear combinations of
interest. I think the following thirteen items are a complete list:
Linear polarization angle 1/2 Arctan(U,Q)
Linearly polarized intensity Sqrt(Q^2 + U^2)
Elliptically polarized intensity Sqrt(Q^2 + U^2 + V^2)
Unpolarised intensity I - Sqrt(Q^2 + U^2 + V^2)
Circularly polarized intensity |V|
Fractional Q Q/I
Fractional U U/I
Fractional V V/I
Fractional linear polarization Sqrt(Q^2 + U^2) / I
Fractional elliptical polarization Sqrt(Q^2 + U^2 + V^2) / I
Fractional circular polarization |V| / I
Fractional unpolarized emission 1 - Sqrt(Q^2 + U^2 + V^2) / I
undefined polarization ---
Some of these (e.g. |V| and |V|/I) may not be needed but are included
to ensure this issue will not have to be re-visited in the future.
Thhe most useful of these are assigned "STOKES" codes by AIPS, viz:
5 => Linearly polarized intensity (pace "Going AIPS" p.5-6 which says
"Percent polarization" in error)
6 => Fractional polarization
7 => Polarization position angle
AIPS also uses STOKES 0 => beam, 8 => Spectral index and 9 => Optical
depth, but these seem inappropriate definitions (all of these may in
general need polarization labels as well). These codes are written to FITS
headers by AIPS.
"Once FITS always FITS" would require that we avoid using codes 0, 8, 9
and either adopt the existing AIPS usage for codes 5,6,7 (if not rendered
ambiguous by the usage of oteher fits writers) or choose new unambiguous
codes (e.g. starting at 10 or 100) for the above set of eleven.
What do people think, and what is the best way of going about (eventually)
getting a formal ruling?
regards,
Paddy Leahy
======================================================
Dr J. P. Leahy, Jodrell Bank Centre for Astrophysics,
Current address: Osservatorio Astronomico di Trieste
INAF, Via GB Tiepolo 11, 34143 Trieste, Italy
Tel.+39 040 3199160 Fax +39 040 309418
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