Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-24T20:57:39.089Z Has data issue: false hasContentIssue false
  • English
  • Français

What Should We Do to Know More About Chromospheres and Coronae of Stars?

Published online by Cambridge University Press:  08 February 2017

Richard N. Thomas
Richard N. Thomas*
Affiliation:
Joint Institute for Laboratory Astrophysics, Boulder, Colorado

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.

Chromospheres-coronas satisfy the last two of the proposed classification schemes: inadequacy of the classical atmosphere (CA) model to represent observations and a priori rejection of the CA model So we survey the question of what is required for more knowledge from the standpoint of asking what conceptual modifications will increase knowledge and what new observations are required. We stress that continued progress requires a continual interchange of ideas between the solar situation and the range of stellar situations.

Keywords

chromosphercoronclassical atmosphere model
Type
Part C. Chromospheres and Coronae of Stars
Information
International Astronomical Union Colloquium , Volume 2: Spectrum Formation in Stars With Steady-State Extended Atmospheres , August 1970 , pp. 259 - 282
Copyright
Copyright © 1970

References

Billings, D. E. 1966, A Guide to the Solar Corona, Academic Press.Google Scholar
Cayrel, R. 1963, Cr. Ac. Sci. Paris, 257, 3309.Google Scholar
Gebbie, K. B. and Thomas, R. N. 1968, Ap. J. 154, 285.CrossRefGoogle Scholar
Gebbie, K. B. and Thomas, R. N. 1968, Proceedings of the Symposium on Wolf-Rayet Stars, National Bureau of Standards Special Publication 307.Google Scholar
Hanbury Brown, R. 1968, in Gebbie, K. B. and Thomas, R. N., Proceedings of the Symposium on Wolf-Rayet Stars, National Bureau of Standards Special Publication 307, p. 79.Google Scholar
IAU, 1957, Joint Discussion on Tubulence in STellar Atmospheres, Transactions of the IAU, 1955, IX, 727, Cambridge University Press.Google Scholar
Jordan, S. D. 1969a, in press, Ap. J., 1969b, in press, Ap. J., 1968, Thesis, University of Colorado.Google Scholar
Kuhi, L. V. 1968, in Gebbie, K. B. and Thomas, R. N., Proceedings of the Symposium on Wolf-Rayet Stars, National Bureau of Standards Special Publication 307, p. 103.Google Scholar
Morton, D. C. 1967, Ap. J. 147, 1017.CrossRefGoogle Scholar
Parker, E. N. 1963, Interplanetary Dynamical Processes, Interscience Publishers Google Scholar
Pecker-Wimel, C. and Thomas, R. N. 1963, Ap. J. 137, 967.CrossRefGoogle Scholar
Redman, R. O. 1942, MNRAS 102, 134.CrossRefGoogle Scholar
Stecher, T. P. and West, D. K. 1968, in Gebbie, R. B. and Thomas, R. N. , Proceedings of the Symposium on Wolf-Rayet Stars, National Bureau of Standards Special Publication 307, p. 65.Google Scholar
Thomas, R. N. 1948, Ap. J. 108, 130.CrossRefGoogle Scholar
Thomas, R. N. 1961, Proceedings of the Fourth Symposium on Cosmical Gas Dynamics, Supp. to Nuovo Cimento XXII.Google Scholar
Thomas, R. N. and Athay, R. G. 1961, Physics of the Solar Chromosphere, Interscience Publishers.CrossRefGoogle Scholar
Thomas, R. N. 1967, Proceedings of the Fifth Symposium on Cosmical Gas Dynamics, Academic Press.Google Scholar