Hostname: page-component-848d4c4894-nmvwc Total loading time: 0 Render date: 2024-06-17T17:21:24.290Z Has data issue: false hasContentIssue false

Visibility Functions of Solar and Stellar Irradiance Variations

Published online by Cambridge University Press:  12 April 2016

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

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 calculated visibility functions of intensity fluctuations due to adiabatic waves in a realistic model of a non-grey, stratified atmosphere in LTE. The results for different optical wavelengths λ and their angular dependence are discussed; moreover, a method for selecting various low-degree p-modes from observations of spectral irradiance fluctuations at different λ including the UV is suggested.

Type
Part 2. Poster Papers
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
Toutain, T., & Gouttebroze, P. 1993, A&A, 268, 309 Google Scholar
Vernazza, J.E., Avrett, E.H., & Loeser, R. 1981, ApJS, 45, 635 CrossRefGoogle Scholar
Zhugzhda, Y.D., Dzhalilov, N.S., & Staude, J. 1993, A&A, 278, L9 Google Scholar