Abstract
We show that the turbulent viscosity forces acting on photospheric meridional currents could cause the solar photosphere to be oblate by more than \ifmmode\pm\else\textpm\fi{}70 km. Although the sign of the effect is undetermined, this might remove the alleged discrepancy in Einstein's prediction for the perihelion advance of Mercury.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
