Search for solar G modes
Despite theoretical predictions on the existence of solar gravity oscillations (g modes), their detection is still marginal. The main reasons are their frequencies, nu less than 0.2 mHz, and amplitudes of less than 10 cm/s. However, because these modes are extremely sensitive to the physical conditions in the very deep sun, they can give detailed
Palle, P. L. et al.
Fecha de publicación:
0
1987