Bibcode
Vázquez Ramió, H.; Mathur, S.; Régulo, C.; García, R. A.
Bibliographical reference
Journal of Physics: Conference Series, Volume 271, Issue 1, pp. 012056 (2011).
Advertised on:
1
2011
Citations
5
Refereed citations
5
Description
CoRoT and Kepler missions are collecting data of solar-like oscillating
stars of unprecedented quality. Moreover, thanks to the length of the
time series, we are able to study their seismic variability. In this
work we use numerical simulations based on the last 3 solar cycles to
analyze the light curves as a function of the line-of-sight inclination
angle. These preliminary results showed that the direct observation of
the light curve can induce some bias in the position of the maximum of
the cycle.
Related projects
Helio and Astero-Seismology and Exoplanets Search
The principal objectives of this project are: 1) to study the structure and dynamics of the solar interior, 2) to extend this study to other stars, 3) to search for extrasolar planets using photometric methods (primarily by transits of their host stars) and their characterization (using radial velocity information) and 4) the study of the planetary
Savita
Mathur