Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-26T04:55:16.427Z Has data issue: false hasContentIssue false
  • English
  • Français

Time-Latitude Prominence and the Green Corona Distribution Over the Solar Activity Cycle

Published online by Cambridge University Press:  12 April 2016

M. Minarovjech ,
M. Rybanský  and
V. Rušin
M. Minarovjech
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 05960 Tatranská Lomnica, Slovakia
M. Rybanský
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 05960 Tatranská Lomnica, Slovakia
V. Rušin
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 05960 Tatranská Lomnica, Slovakia

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.

We present a distribution of prominences over the solar cycle activity. There are found both polar and equatorial branches of prominences that migrate in opposite directions. Prominences of the high-latitude crown migrate, starting in the minimum of the cycle, towards the poles, which they reach at the maximum of the cycle and then decay. The equatorward-migrating branch of prominences appears also in the minimum of the cycle at mid-latitudes and disappears at the end of the cycle. The distribution of the prominences is compared with a time-latitudinal distribution of the green corona. It is assumed that the polar branches in cycle 23 will reach the poles in 2002 (the north pole) and 2003 (the south one), respectively.

Type
Global Patterns
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 484 - 487
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Altrock, R.C., Rybanský, M., Rušin, V. and Minarovjech, M. 1997, Contrib. Astron. Obs. Skalnaté Pleso, 27, 25 Google Scholar
Bumba, V. Rušin, V. and Rybanský, M. 1990, Bull. Astron. Inst. Czechosl. 41, 253 Google Scholar
Dermendjiev, V.N., Stavrev, K.Y., Rušin, V. and Rybanský, M. 1994, A&A, 281, 241 Google Scholar
Howard, R. and LaBonte, B.J. 1980 ApJ, 239, L33 Google Scholar
Makarov, V. and Sivaraman, K.R. 1989, Solar Phys., 123, 367 Google Scholar
Minarovjech, M., Rybanský, M. and Rušin, V. 1997, Solar Phys., 177, 357 Google Scholar
Rušin, V., uRybanský, , Dermendjiev, V. and Stavrev, K.Ya. 1988, Contrib. Astron. Obs. Skalnaté Pleso 17, 63 Google Scholar
Secchi, P.A. 1872, Die Sonne, BraunschweigGoogle Scholar
Tandberg-Hanssen, E. 1974, Solar Prominences, D. Reidel, Dordrecht, Holland Google Scholar
Waldmeier, M. 1973, Solar Phys., 28, 389 Google Scholar