Quantum theory of line formation in a magnetic field
โ Scribed by Egidio Landi Degl'innocenti; Maurizio Landi Degl'innocenti
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 489 KB
- Volume
- 27
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
The transfer equations for the Stokes parameters in the presence of magnetic field and under the hypothesis of LTE are derived in an original way by the use of density matrix techniques.
The results are substantially the same as those previously obtained by other authors. We finally compare our results to the previous ones in order to clarify some discrepancies still present in the literature.
Solar Physics 27 (1972) 319-329. All Rights Reserved Copyright 9 1972 by D. Reidel Publishing Company, Dordrecht-Holland * The reason of our statements on page 322 is that the infinite terms of the form <ks, k', fl Q fka, i) would contribute to the right-hand side of ( 7) with a quantity proportional to 8(v' + v0) and those (finite in number) with k' =ks, 2 with quantities proportional to 8(v0 +v) and to P/(vo +v). * This definition is the same as the operational one given by Shurcliff (1962) except for a factor V'2 in U and V.
๐ SIMILAR VOLUMES
The formation of a Zeeman-multiplet by noncoherent scattering and true absorption in a Milne-Eddington atmosphere is considered assuming a homogeneous magnetic field and complete depolarization of the atomic line levels. The transfer equation for the Stokes parameters is transformed into a scalar in
Theoretical line contours calculated for fixed values of the line constants and a given model atmosphere show an increase of the Stokes parameters Q, U, and V but a decrease of I if the portion of non-coherent scattering increases. These effects increase from the centre of the solar disk to the limb