Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-26T03:26:35.690Z Has data issue: false hasContentIssue false
  • English
  • Français

Oscillatory modes of energy transport in solar magnetic regions∗

Published online by Cambridge University Press:  14 August 2015

R. E. Danielson  and
B. D. Savage
R. E. Danielson
Affiliation:
Princeton University Observatory, Princeton, N.J., U.S.A.
B. D. Savage
Affiliation:
Princeton University Observatory, Princeton, N.J., U.S.A.

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.

It appears that it is necessary to look for oscillatory (i.e. overstable) instabilities as the cause of energy transport in sunspots. Making use of recent calculations on the hydromagnetic stability of thermally unstable layers with open boundary conditions, it is found that oscillatory modes can occur in the interior of sunspots. Some possible consequences of these oscillatory modes are discussed.

Type
Part II: Theoretical Aspects
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 112 - 125
Copyright
Copyright © Reidel 1968 

References

Beckers, J., Schröter, E. (1967) private communication.Google Scholar
Böhm, K. H. (1963) Astrophys. J., 137, 881.CrossRefGoogle Scholar
Böhm-Vitense, E. (1958) Z. Astrophys., 46, 108.Google Scholar
Bray, R., Loughhead, R. (1959) Austr. J. Phys., 12, 320.CrossRefGoogle Scholar
Brückner, G. (1965) in I.A.U. Symposium No. 22: Solar and Stellar Magnetic Fields, Ed. by Lüst, R., North-Holland Publ. Co., Amsterdam, p. 293.Google Scholar
Chandrasekhar, S. (1961) Hydrodynamic and Hydromagnetic Stability, Oxford University Press, London.Google Scholar
Chitre, S. (1963) Mon. Not. R. astr. Soc., 126, 431.CrossRefGoogle Scholar
Danielson, R. E. (1961) Astrophys. J., 134, 289.CrossRefGoogle Scholar
Danielson, R.E. (1964) Astrophys. J., 139, 45.CrossRefGoogle Scholar
Danielson, R.E. (1965) in I.A.U. Symposium No. 22: Solar and Stellar Magnetic Fields, Ed. by Lüst, R., North-Holland Publ. Co., Amsterdam, p. 315.Google Scholar
Danielson, R.E. (1966) in Convegno Sulle Machie Solare, Ed. by Barbera, (Firenze).Google Scholar
Deinzer, W. (1965) Astrophys. J., 141, 548.CrossRefGoogle Scholar
Elsässer, H., Fricke, K. (1965) in I.A.U. Symposium No. 22: Solar and Stellar Magnetic Fields, Ed. by Lüst, R., North-Holland Publ. Co., Amsterdam, p. 297.Google Scholar
Elste, G. (1963) J. Quant. Spect. Rad. Trans., 3, 185.CrossRefGoogle Scholar
Howard, R. (1958) Astrophys. J., 127, 108.CrossRefGoogle Scholar
Kato, S. (1966) P.A.S.J., 18, 201.Google Scholar
Marik, M. (1966) Soviet Astr. - A.J., 10, 315.Google Scholar
Musman, S. (1967) Astrophys. J., 149, 201.CrossRefGoogle Scholar
Savage, B.D. (1967) , Princeton University.Google Scholar
Spiegel, E. A., Veronis, G. (1960) Astrophys. J., 131, 442.CrossRefGoogle Scholar
Vitense, E. (1953) Z. Astrophys., 32, 135.Google Scholar
Weiss, N. O. (1964) Proc. Roy. Soc., A256, 99.Google Scholar
Yun, H.S. (1967) private communication.Google Scholar