Published August 1978 | Version v1
Journal article Metadata-only

The origin of running penumbral waves

Creators

  • 1. Sussex Univ., Brighton (UK)

Description

Numerical experiments on axisymmetric convection with a magnetic field display solutions in which steady convection concentrates the field into a strong central rope. Subsequently, oscillations develop within the rope; this process models the formation of a sunspot with running penumbral waves. (author)

Additional details

Identifiers

DOI
10.1093/mnras/184.1.49p;

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
184
Journal Issue
1
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
49P-52P
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
9413119
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CONVECTION; MAGNETIC FIELDS; NUMERICAL SOLUTION; OSCILLATION MODES; OSCILLATIONS; PHOTOSPHERE; STAR MODELS; SUNSPOTS; WAVE PROPAGATION
Descriptors DEC
ATMOSPHERES; ENERGY TRANSFER; HEAT TRANSFER; MATHEMATICAL MODELS; SOLAR ACTIVITY; SOLAR ATMOSPHERE

Optional Information

Notes
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