Detection of periodic signatures in the solar power spectrum On the track of l=1 gravity modes
In the present work we show robust indications of the existence of g modes in the Sun using 10 years of GOLF data. The present analysis is based on the exploitation of the collective properties of the predicted low-frequency (25 to 140 microHz) g modes: their asymptotic nature, which implies a quasi equidistant separation of their periods for a
García, R. A. et al.
Fecha de publicación:
10
2006