Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-14T05:38:40.716Z Has data issue: false hasContentIssue false

Hydromagnetic Structure at the Boundary of a Supergranule

Published online by Cambridge University Press:  25 April 2016

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

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
Copyright
Copyright © Astronomical Society of Australia 1971

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Livingston, W. and Harvey, J., Solar Phys., 10, 294 (1970).Google Scholar
2 Giovanelli, R. G., Proc. ASA, 1, 363 (1970).Google Scholar
3 Frazier, E. N., Solar Phys., 14, 89 (1970).CrossRefGoogle Scholar
4 Beckers, J. M. and Schröter, E. H., Solar Phys., 4, 142 (1968).CrossRefGoogle Scholar
5 Chapman, G. A. and Sheeley, N. R., Solar Phys., 5, 442 (1968).Google Scholar
6 Harvey, J. and Livingston, W., Solar Phys., 10, 283 (1970).Google Scholar
7 Lundquist, S., Phys. Rev., 83, 307 (1951).CrossRefGoogle Scholar
8 Parker, E. N., Ap. J., 138, 552 (1963).Google Scholar
9 Weiss, N. O., Proc. Roy. Soc. A, 293, 310 (1966).Google Scholar
10 Unno, W., Ap. J., 126, 259 (1957).CrossRefGoogle Scholar
11 Uchida, Y., Publ. Astr. Soc. Japan, 21, 128 (1969).Google Scholar