Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-30T18:59:53.120Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution of the Magnetic Field Configuration in an Active Region

Published online by Cambridge University Press:  14 August 2015

Dennis L. Schatz
Dennis L. Schatz*
Affiliation:
CSIRO National Standards Laboratory, Division of Physics, Sydney, Australia

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.

Described and discussed is the evolution of the magnetic field configuration in an Active Region from observations made with high time resolution.

Type
Part III: Observations of Sunspot and Active Region Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 243 - 248
Copyright
Copyright © Reidel 1971 

References

Chapman, G. A. and Sheeley, N. R.: 1969, Solar Phys. 9, 347.Google Scholar
Giovanelli, R. G.: 1967, Proc. Astron. Soc. Australia 1, 39.CrossRefGoogle Scholar
Giovanelli, R. G.: 1970, Proc. Astron. Soc. Australia 1, 363.CrossRefGoogle Scholar
Leighton, R. B.: 1959, Astrophys. J. 130, 366.CrossRefGoogle Scholar
Ramsay, J. V.: 1967, Proc. Astron. Soc. Australia 1, 66.CrossRefGoogle Scholar
Ribes, E.: 1969, Astron. Astrophys. 2, 316.Google Scholar
Schatz, D.: 1970, Proc. Astron. Soc. Australia 1, 371.CrossRefGoogle Scholar
Sheeley, N. R.: 1968, Solar Phys. 5, 442.Google Scholar