Convective instability in the solar envelope

Research paper by D. Narasimha, S. K. Pandey, S. M. Chitre

Indexed on: 01 Dec '80Published on: 01 Dec '80Published in: Journal of Astrophysics and Astronomy


The characteristics of the most unstable fundamental mode and the first harmonic excited in the convection zone of a variety of solar envelope models are shown to be in reasonable agreement with the observed features of granulation and supergranulation.