Variations of the solar granulation motions with height using the GOLF/SoHO experiment
Context: Below 1 mHz, the power spectrum of helioseismic velocity measurements is dominated by the spectrum of convective motions (granulation and supergranulation) and it is difficult to detect the low-order acoustic modes and gravity modes. Aims: We attempt to understand more clearly the behavior of solar granulation as a function of observing
Lefebvre, S. et al.
Fecha de publicación:
11
2008