Effect of line-of-sight inclinations on the observation of solar activity cycle: Lessons for CoRoT & Kepler

Bibcode
2011JPhCS.271a2056V
DOI
10.1088/1742-6596/271/1/012056
Vázquez Ramió, H.; Mathur, S.; Régulo, C.; García, R. A.
Referencia bibliográfica

Journal of Physics: Conference Series, Volume 271, Issue 1, pp. 012056 (2011).

Fecha de publicación:
1
2011
Número de autores
4
Número de autores del IAC
0
Número de citas
5
Número de citas referidas
5
Descripción
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.
Proyectos relacionados
Helio y Astroseismología
Sismología Solar y Estelar y Búsqueda de Exoplanetas
Los objetivos principales de este proyecto son: 1) estudiar la estructura y la dinámica del interior solar, 2) ampliar este estudio a otros tipos de estrellas y 3) buqueda de planetas extrasolares utilizando métodos fotométricos y su caracterización con información complementaria (espectrometría). Para alcanzar el primer objetivo, utilizamos la
Savita
Mathur
En ejecución
Tipo
Sin árbitro
Física estelar e interestelar (FEEI)

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