𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Line formation in the presence of a magnetic field II. Source functions

✍ Scribed by H. Domke


Publisher
Springer
Year
1973
Tongue
English
Weight
675 KB
Volume
7
Category
Article
ISSN
0571-7256

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Quantum theory of line formation in a ma
✍ Egidio Landi Degl'innocenti; Maurizio Landi Degl'innocenti πŸ“‚ Article πŸ“… 1972 πŸ› Springer 🌐 English βš– 489 KB

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 res

On the mean depth of line formation in a
✍ JΓΌrgen Staude πŸ“‚ Article πŸ“… 1972 πŸ› Springer 🌐 English βš– 356 KB

Probability interpretation of radiative transfer is used to calculate the contribution of different layers of the solar atmosphere to the emergent intensity. Generally the mean depths of line formation increase with increasing intensity; this is valid also for arbitrarily polarized constituents of a

The laminar plume above a line heat sour
✍ Gray, Donald D. πŸ“‚ Article πŸ“… 1977 πŸ› Springer 🌐 English βš– 724 KB

The dynamics of a buoyant plume rising above a horizontal line heat source in a transverse, horizontal magnetic field is investigated. Similarity is shown to occur when the magnetic field strength varies as the -2/5 power of vertical distance from the source. The plume depends on two parameters -the