GHST CRYPTOBITCOIN PAPER TRADING

Velocity field illustrating the turbulent convective motions close to the surface of a spherical shell via the use of 3D numerical simulations.

Schematic depiction of various meridional circulation profiles, a crucial component of flux transport dynamo models, is a topic of extensive research.

Subsurface velocity fields illustrating the complex large-scale motions near active regions.
Figure: Deborah A. Haber, 2001

Science On a Sphere exhibit at The Lawrence Hall of Science, displays data, images, and animations to science center visitors from around the world.