Solar
Magnetic Flux Tubes
Solar Magnetic Flux Tubes are magnetic field concentrations near the
surface of the sun. Because of their close relation to their much
larger cousins, sun spots, they are of great interest to researchers.
Volume visualization is used here to study the formation and collapse
of the flux tubes as they evolve over time.
TIDI
Measurements of Upper Atmosphere Dynamics
The TIDI instrument collects upper atmosphere wind velocity data as the
TIMED satelite orbits the globe. The data shown on the surface of the
globe is a hyperslice in time and space depicting upper atmosphere wind
speeds.
Penetrative
Turbulent Convection in a Compressible Gas
The outer third of the Sun's radius is convectively unstable. Turbulent
motions from this region may penetrate into stable layers below, mixing
temperature, momentum and chemicals.