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Hydromagnetic Structure at the Boundary of a Supergranule

Published online by Cambridge University Press:  25 April 2016

E. Ribes  and
W. Unno
E. Ribes
Affiliation:
CSIRO Division of Physics, National Standards Laboratory, Sydney
W. Unno
Affiliation:
CSIRO Division of Physics, National Standards Laboratory, Sydney
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Extract

We shall examine the question of whether the concentration of magnetic field, the downward motion and the temperature excess observed at the boundaries of supergranules can be interpreted consistently in terms of a steady flow along the magnetic lines of force. Before doing so, however, we shall first consider the development of the magnetic configuration driven by a supergranular convection overshooting into the photosphere.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 1 , July 1971 , pp. 54 - 55
Copyright
Copyright © Astronomical Society of Australia 1971

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References

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