Hostname: page-component-745bb68f8f-g4j75 Total loading time: 0 Render date: 2025-01-12T13:01:21.937Z Has data issue: false hasContentIssue false
  • English
  • Français

An Analytic Theory of Adiabatic p-modes in the Atmospheres of the Sun and Sun-like Stars

Published online by Cambridge University Press:  12 April 2016

Namig S. Dzhalilov  and
Jürgen Staude
Namig S. Dzhalilov
Affiliation:
IZMIR RAN, Troitsk, Moscow Region, 142092Russia
Jürgen Staude
Affiliation:
Astrophysikalisches Institut Potsdam, Sonnenobservatorium ‘Einstein-Turm’, Telegrafenberg, D-14473 Potsdam, Germany

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.

An analytic theory of resonant transmission has been used to study adiabatic, non-vertical oscillations in a realistic model of the solar or a stellar atmosphere and subphotosphere. Basic observed features of solar p-modes can be explained in this way.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 449 - 450
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Dzhalilov, N.S., Zhugzhda, Y.D., & Staude, J. 1994, A&A, 291, 1001 Google Scholar
Staude, J., Dzhalilov, N.S., & Zhugzhda, Y.D. 1994, Solar Phys., 152, 227 CrossRefGoogle Scholar
Zhugzhda, Y.D., Dzhalilov, N.S., & Staude, J. 1993, A&A, 278, L9 Google Scholar