Global fitting of power spectra of solar-like stars

Details Global fitting of power spectra of solar-like stars Global fitting of power spectra of solar-like stars

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.538..373n&link_type=abstract

In: Second Eddington Workshop: Stellar structure and habitable planet finding, 9 - 11 April 2003, Palermo, Italy. Edited by F. F

Other

Stars: Solar-Like, Stars: Pulsations, Method: Global Fitting

Scientific paper

Helioseismology has been able to provide the internal structure of the Sun and its dynamics. These inferences have been made possible by inverting the frequencies and rotational splitting of the p-mode oscillations. Thanks to asteroseismology, similar results can now be obtained for stars other than the Sun. For this purpose, we are developing a numerical code for global fitting of power spectra. The code is currently developed and tested on full-disk integrated solar data obtained with the SOHO/LOI instrument. It will then be applied to synthetic data from the hare-and-hound exercises of COROT. The final goal is to apply the technique to data of solar-like stars obtained with the COROT and Eddington satellites to infer the internal structure and dynamics of those stars.

Affiliated with

Also associated with

No associations

Rating

Global fitting of power spectra of solar-like stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Global fitting of power spectra of solar-like stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Global fitting of power spectra of solar-like stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1550197