}?>
By Joining you agree to MachPrinciple's Terms and Conditions and Privacy Policy
Click to Login
Please check your email. A registration confirmation link will be sent to your mailbox..
A registration confirmation link has been sent to your email. Please check your email and finish the registration process.
Search a Conference through our dedicated search page
Understanding stellar convection is of crucial importance to many fields of stellar astrophysics. For example, the generation and maintenance of differential rotation and large-scale magnetic fields in stars rely on turbulent convection. However, mounting evidence suggests that our understanding of stellar convection is much more incomplete than previously thought. We bring together experts in three-dimensional convection simulations, helio- and asteroseismology, and theoreticians working on replacing the mixing length concept to present the latest developments and to address open problems in the field.