Issue |
A&A
Volume 476, Number 2, December III 2007
|
|
---|---|---|
Page(s) | 665 - 674 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361:20077980 | |
Published online | 23 October 2007 |
The Hanle effect
Decomposition of the Stokes parameters into irreducible components
Laboratoire Cassiopée (CNRS), Université de Nice, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex 4, France e-mail: frisch@obs-nice.fr
Received:
31
May
2007
Accepted:
14
September
2007
Context.It has been shown for the weak-field Hanle effect that the Stokes parameters I, Q, and U can be represented by a set of six cylindrically symmetrical functions. The proof relies on azimuthal Fourier expansions of the radiation field and of the Hanle phase matrix. It holds for a plane-parallel atmosphere and scattering processes that can be described by a redistribution matrix where redistribution in frequency is decoupled from angle redistribution and polarization.
Aims.We give a simpler and more general proof of the Stokes parameter
decomposition using powerful new tools introduced for polarimetry,
in particular the Landi Degl'Innocenti spherical tensors .
Methods.The elements of the Hanle phase matrix are written as a sum of terms
that depend separately on the magnetic field vector and the
directions and
of the incoming and
scattered beams. The dependence on
and
is expressed in terms of the spherical tensors
where i refers to the Stokes parameters
(
). A multipolar expansion in terms of the
is then established for the source term in the
transfer equation for the Stokes parameters.
Results.We show that the Stokes parameters have a multipolar expansion that
can be written as (
,
)
where the
are nine cylindrically symmetrical, irreducible
tensors, θ being the inclination of
with respect
to the vertical in the atmosphere. The proof is generalized to
frequency-dependent phase matrices. It is applied both to partial
frequency redistribution with angle-averaged scalar frequency
redistribution functions and to complete frequency redistribution
with the Hanle effect in the line core and Rayleigh scattering in the
wings. Non-LTE transfer equations for the
and integral
equations for the associated source functions
are
established. Formal vectors and matrices constructed with
,
, and
are introduced in order to present
the results in a compact matrix notation. In particular, a simple
factorized form is proposed for the Hanle phase matrix.
Key words: line: formation / polarization / magnetic fields / radiative transfer
© ESO, 2007
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