Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-26T19:56:46.338Z Has data issue: false hasContentIssue false
  • English
  • Français

Boundary Fitting Problems Associated with Coronal Magnetic Models

Published online by Cambridge University Press:  25 May 2016

Kenneth H. Schatten
Kenneth H. Schatten*
Affiliation:
Victoria University, Wellington, New Zealand

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The calculation of coronal magnetic fields was first suggested by Gold (1958). Altschuler and Newkirk (1969) and Newkirk et al. (1968) used a Legendre polynomial fit to the photospheric observations of magnetic fields whereas Schatten (1968) with Wilcox and Ness (Schatten et al., 1969) use a magnetic monopole fit, first incorporated by Schmidt (1964).

Type
Part I Magnetic Structure Responsible for Coronal Disturbances
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 89 - 91
Copyright
Copyright © Reidel 1974 

References

Altschuler, M. D. and Newkirk, G. Jr.: 1969, Solar Phys. 9, 131.Google Scholar
Gold, T.: 1958, in Lehnert, B. (ed.), ‘Electromagnetic Phenomena in Cosmical Physics’, IAU Symp. 6, 275.Google Scholar
Newkirk, G. Jr., Altschuler, M. D., and Harvey, T. W.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, 379.Google Scholar
Schatten, K. H.: 1968, , Univ. of Calif. Berkeley.Google Scholar
Schatten, K. H., Wilcox, J. M., and Ness, N. F.: 1969, Solar Phys. 6, 442.Google Scholar
Schmidt, H. O.: 1964, in Hess, W. (ed.), AAS-NASA Symposium on Physics of Solar Flares, NASA SP-50, p. 107.Google Scholar