Published January 1978
| Version v1
Journal article
On the dynamic interaction between magnetic fields and convection
Description
A simple two-dimensional model of convection in an electrically conducting Boussinesq fluid with an externally imposed magnetic field has been investigated in a series of numerical experiments. Convection is driven by horizontal gradients in an imposed temperature field which is unaffected by the motion. The transition from a kinematic to a dynamic regime is studied: magnetic flux is concentrated into ropes and the maximum field strength depends on the ratio of the viscous and magnetic diffusivities. The magnetic energy density in the ropes is unrelated to, and may be much greater than, the kinetic energy density outside. These results are relevant to the interaction between small-scale magnetic fields and photospheric in the Sun. (author)
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 182
- Journal Issue
- 2
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 189-208
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 9374945
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CONVECTION; ELECTRIC CONDUCTIVITY; FLUIDS; MAGNETIC FIELDS; MAGNETIC FLUX; PHOTOSPHERE; SOLAR GRANULATION; STAR MODELS; SUN
- Descriptors DEC
- ATMOSPHERES; ELECTRICAL PROPERTIES; ENERGY TRANSFER; HEAT TRANSFER; MATHEMATICAL MODELS; PHYSICAL PROPERTIES; SOLAR ACTIVITY; SOLAR ATMOSPHERE; STARS
Optional Information
- Notes
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