Issue |
A&A
Volume 461, Number 1, January I 2007
|
|
---|---|---|
Page(s) | 1 - 10 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361:20042232 | |
Published online | 26 September 2006 |
Polarization properties of resonance scattering in molecular bands
The intermediate (a-b) coupling regime
1
Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, Largo E. Fermi 2, 50125 Firenze, Italy
2
Universität-Sternwarte Göttingen, Geismarlandstr. 11, 37083 Göttingen, Germany e-mail: landie@arcetri.astro.it
Received:
22
October
2004
Accepted:
25
August
2006
The polarimetric properties of the phenomenon of resonance scattering
in molecular bands are analyzed in detail for the general case where both the
lower and upper electronic states of the molecule are described in the
coupling scheme intermediate between Hund's cases (a) and (b). A semi-analytical
expression is derived for the line polarizability factor in the special
case where atomic polarization is neglected in the lower electronic state, and
particular attention is devoted to clarifying the role played by the phenomenon
of Λ-doubling, which turns out to be particularly relevant in the case
of transitions. The expression for the line polarizability
factor is derived for both cases where the energy eigenvectors are expressed
as a linear combination of the eigenvectors relative to Hund's case (a)
and of those relative to Hund's case (b). Such expressions are then combined
with the corresponding expressions of the Einstein coefficient and of the
Landé factors to obtain an estimate of the linear polarization signals to
be expected in molecular bands observed at the solar limb either in the
quiet atmosphere or in magnetic regions. Illustrative results are shown for
the bands of MgH and of C2 around 5100 Å.
Key words: molecular processes / scattering / polarization
© ESO, 2006
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