Published March 1979
| Version v1
Journal article
The origin of supergranulation and giant cells in the solar convective zone
Description
In the standard model of the solar convective zone, turbulent eddies transport entropy rather than temperature. The authors consider the turbulent mean field equations for the convective zone, including entropy transport, and show that the zone can be unstable to larger scale motion which is identified with the supergranulation and giant cells. (Auth.)
Additional details
Publishing Information
- Journal Title
- Sol. Phys.
- Journal Volume
- 61
- Journal Issue
- 2
- Series
- Sol. Phys.
- Journal Page Range
- 247-250
- ISSN
- 0038-0938
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 10483561
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CONVECTIVE INSTABILITIES; ENTROPY; FIELD EQUATIONS; SOLAR ATMOSPHERE; SOLAR GRANULATION; STAR MODELS; SUN; TURBULENCE
- Descriptors DEC
- ATMOSPHERES; EQUATIONS; INSTABILITY; MAIN SEQUENCE STARS; MATHEMATICAL MODELS; PHYSICAL PROPERTIES; PLASMA INSTABILITY; SOLAR ACTIVITY; STARS; THERMODYNAMIC PROPERTIES