The majority of the loops are arranged in long rows or arcades, which frequently cover a large fraction of the surface.
Nice, like mitochondria.
http://history.nasa.gov/EP-177/ch3-3.htmlGreat link Sparko.
Perhaps the Sun's most remarkable magnetic features are the coronal transients. These objects were discovered by the seventh Orbiting Solar Observatory satellite (OSO-7) and later were studied intensively by Skylab. A typical transient begins as a gigantic bubble that appears near the solar surface and flies out through the corona at a velocity of hundreds of kilometers per second. These transients usually are caused by solar flares or by the eruption of a type of solar prominence known as a cool loop. The bubbles, consisting of high temperature plasma, carry along magnetic fields from the lower corona and disrupt the upper corona as they expand outward.
The temperatures and densities of coronal holes are much lower than those of other parts of the corona. Investigations show that in the holes, the magnetic field has no loops, but extends directly out into the solar wind. [or in?] We do not yet know how and why coronal holes form, but we do know that they are a major source of the solar wind. Two apparently permanent coronal holes exist at the north and south poles of the Sun, and it may be that much of the solar wind that leaves the Sun originates in these two polar coronal holes
Bubbles and holes. Are we seeing a pattern here?
Parker explained, that its gas is constantly evaporating away from the Sun at supersonic speed.
Either they need to take another look at solar transmissions, or we need to take another look at terrestrial evaporation...
Overall, the site definitely shows NASA getting electricity, and much better illumination for the money.
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