We present 2-D numerical models of quiescent solar prominences with normal magnetic polarity. These models represent an extension to the classical Kippenhahn-Schltiter model in that the prominence is treated as having finite width and height and the external coronal field is matched smoothly to the
The effect of shear on numerical models of quiescent normal-polarity prominences
โ Scribed by R. A. S. Fiedler; A. W. Hood
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 693 KB
- Volume
- 146
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
A model of a quiescent prominence with nonparallel structural elements, based on a study of the K Ca ยง line fine structure of two quiescent prominences. The dependences of the radial velocities on the height found for the structural elements making up the prominence (Gigolashvili and Zhugzhda, 1982)
## Summa~ The effect of the presence of a free surface on the behaviour of shear-modified internal waves is investigated. In all cases, the qualitative behaviour with varying Richardson number is similar to that in the case of a rigid upper boundary. The quantitative differences are shown to be sm
## Abstract In this paper we consider the following nested random effect model magnified image where the ฮฑ~__i__~'s, the ฮฒ~__ij__~'s and the __e__~__ijk__~ are independent random variables. By assuming that these variables follow a mixture of two normal densities, we study the effects of departure