Published July 1, 1979 | Version v1
Journal article

Sunspots and the physics of magnetic flux tubes. V. Mutual hydrodynamic forces between neighboring tubes

Creators

  • 1. Department of Physics and Department of Astronomy and Astrophysics, University of Chicago

Description

The mutual hydrodynamic forces between parallel cylinders in a moving fluid are illustrated through several formal examples. Parallel tubes in a uniform flow are attracted or repelled depending on whether they are side by side or one ahead of the other, respectively. A pulsating or undulating tube attracts all other neighboring tubes toward itself. These hydrodynamic effects suggest that the separate flux tubes beneath the sunspots exert significant attractive forces on each other

Additional details

Publishing Information

Journal Title
Astrophys. J.
Journal Volume
231
Journal Issue
1
Series
Astrophys. J.
Journal Page Range
270-276
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
11498322
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data
Descriptors DEI
EQUATIONS OF MOTION; FLUID FLOW; HYDRODYNAMICS; MAGNETIC FIELD CONFIGURATIONS; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETOHYDRODYNAMICS; SUNSPOTS
Descriptors DEC
DIFFERENTIAL EQUATIONS; EQUATIONS; FLUID MECHANICS; MECHANICS; SOLAR ACTIVITY