A model for the corona of a spherical star cluster
β Scribed by L. P. Osipkov
- Book ID
- 111502546
- Publisher
- Allerton Press, Inc.
- Year
- 2008
- Tongue
- English
- Weight
- 169 KB
- Volume
- 41
- Category
- Article
- ISSN
- 1063-4541
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π SIMILAR VOLUMES
The hydrodynamic equations for art ideal, inviscid, fully ionized hydrogen gas in a gravitational, but not magnetic, field are solved by an explicit Lax-Wendroff two-step technique using a one-dimensional slab symmetry. Radiation and thermal conductivity are included. The model spans 100000 km start
A coronal index (CI) derived from the limb observations of the 530.3 nm emission corona (green corona) over 1964-1987 was analyzed by the Fourier transform technique (FTT) to find periodicity in this layer of solar atmosphere. As expected, two pronounced periods were indicated: the rotational, about