Up: Stokes parameters of resonance
The angular terms
,
and
are function of the angular coordinates
of an emmetting point on the solar disk; the angular coordinates
of the magnetic field vector (or of the velocity field vector); the scattering angle
and of
(where
is the Larmor angular frequency and
is the lifetime of the upper level of the atomic transition considered). Their expressions are given by the following equations
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(A.1) |
where
 |
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(A.2) |
and
\sin(2\psi) ;
\end{array}$](/articles/aa/full/2002/17/aa1681/img133.gif) |
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(A.3) |
\big[d^2_{22}-d^2_{2-2}\big](\eta)\sin(2\psi) ;
\end{array}$](/articles/aa/full/2002/17/aa1681/img134.gif) |
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(A.4) |
\big[d^2_{22}-d^2_{2-2}\big](\eta)\cos(2\psi) .
\end{array}$](/articles/aa/full/2002/17/aa1681/img135.gif) |
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(A.5) |
The coefficients
are given in Brink & Satchler (1962).
Up: Stokes parameters of resonance
Copyright ESO 2002