Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-23T11:19:44.533Z Has data issue: false hasContentIssue false
  • English
  • Français

Results from Iphir as Guideline for Asteroseismology

Published online by Cambridge University Press:  12 April 2016

Thierry Toutain  and
Claus Fröhlich
Thierry Toutain
Affiliation:
Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center CH-7260 Davos Dorf, Switzerland
Claus Fröhlich
Affiliation:
Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center CH-7260 Davos Dorf, Switzerland

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.

The long uninterrupted observation of the Sun as a star with the IPHIR experiment can be used to set limits to the significance of the determination of p-mode parameters as a function of time and the length of the time series of measurements.

Type
VIII. Asteroseismology: observation
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 713 - 716
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Ehgamberdiev, S., S., Khalikov, M.Lazrek, , E., Fossat, 1991, A&A 253, 252.Google Scholar
Toutain, Th., C., Fröhlich, 1992, A&A 257, 287.Google Scholar