Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-19T06:36:36.504Z Has data issue: false hasContentIssue false
  • English
  • Français

Self-Organization Processes on the Sun: The Heliosynergetics

Published online by Cambridge University Press:  19 July 2016

V. Krishan  and
E.I. Mogilevskij
V. Krishan
Affiliation:
Indian Institute of Astrophysics, Bangalore 560034, India
E.I. Mogilevskij
Affiliation:
Indian Institute of Astrophysics, Bangalore 560034, India

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.

Abstract Non-linear interactions between small fluid elements, magnetized or otherwise, in an energetically open nonlinear system facilitate the formation of large coherent stable structures. This is knwon as self-organization. We interpret solar granulation on all scales and the formation and evolution of some structures in solar active regions to be the result of self-organization processes occuring in a turbulent medium.

Type
IV. Photospheric Flows and Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 125 - 133
Copyright
Copyright © Kluwer 1990 

References

Antia, H.M., Chitre, S.M. and Narasimha, D. 1984, Ap. J. 282, 574–583.CrossRefGoogle Scholar
Bogart, R.S., Gierasch, P.J. and MacAuslan, J.M. 1980, Ap. J. 236, 285–293.Google Scholar
Brandt, P.N. et al. 1988, Nature 335, 238–240.CrossRefGoogle Scholar
Hasegawa, A. 1985, Advances in Physics 34, 1–42.Google Scholar
Hasegawa, A., Kodama, Y. and Watanabe, K. 1981, Phys. Rev. Lett. 47,1525.Google Scholar
Kraichnan, R.H. 1967, Phys. Fluids 10, 1417–1423.Google Scholar
Levich, E. and Tzvetkov, E. 1985, Physics Reports 128, No.1, 1–37.CrossRefGoogle Scholar
Mogilevskij, E.I. 1984 Preprint No.43a (517).Google Scholar
Nelson, G.D. and Musman, S. 1978, Ap.J. 222, L69.CrossRefGoogle Scholar
Parker, E.N. 1979, Cosmical Magnetic Fields, Clarendon Press, Oxford.Google Scholar
Schwarzchild, M. 1975, Ap. J. 195, 137–144.Google Scholar
Simon, G.W. and Leighton, R.B. 1965, Ap. J. 140, 1120–1147.Google Scholar
Spruit, H. 1978, in Magnetic Flux Tubes and Transport of Heat in the Convection Zone of the Sun, Utrecht, Holland.Google Scholar