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What are these images?

This image of the Earth was taken by the Galileo spacecraft at about 6:10 a.m. PST on December 11, 1990. The spacecraft was about 1.3 million miles from the Earth. South America is near the center of the picture, and the white, sunlit continent of Antarctica is below. Picturesque weather fronts are visible in the South Atlantic, lower right. (courtesy of NASA/JPL)
source: UCAR's window to the universe

SOHO Extreme ultraviolet Imaging Telescope (EIT) full-field He II 304 Angstroms. Images from NASA Goddard Space Flight Center [ 2003/12/16 19:19:33 ] He II is formed primarily at 60,000 - 80,000 K.
source: EIT Consortium


Billow Clouds on Mt. Shasta
Billow clouds are created from instability associated with air flows having marked vertical shear and weak thermal stratification. The common name for this instability is Kelvin-Helmholtz instability. These instabilities are often visualized as a row of horizontal eddies aligned within this layer of vertical shear.

Billow clouds are created in the upward branch of each of the eddies if the air within this branch has a high enough relative humidity that, upon lifting, the air parcel reaches saturation. Individual billow clouds generally have life times of a few minutes. The presence of billow clouds provides a visible signal to aviation interests of potentially dangerous turbulence.



Satellite image of sea surface temperature in the Atlantic basin. The warm Gulf Stream is clearly visible. The large scale vortices produced by this flow are an example of two dimensional geophysical turbulence.

Volume rendered image of potential vorticity in a numerical quasi-geostrophic simulation where rotation is slanted at 45 degrees. At the end of the run-down experiment, positive vortices (green) and negative vortices (orange) have merged with each other on each horizontal plane. Like-sign vortices on different planes tend to align with the axis of rotation.

Created by Mark Petersen


One can construct maps of systems that display roll switching phenomena in Rayleigh Benard convection experiments. The figure shows an example of rolls whose axes intersect at angle pi/2-epsilon.

This figure shows some of the extraordinary dynamics for T_1=7, T_3=5, and epsilon=.08 for randomly chosen initial conditions in the fundamental rhombic cell. A normal form expansion about the elliptic fixed point at the intersection of roll axes, can be used to show that the dynamics in that region are generally simple. As we move away from those regions, the motion becomes increasingly chaotic in a three-dimensional sense. This is demonstrated by the blue, light blue, and red orbits.

Created by Paul Mullowney