A snaking, extended filament of solar material currently lies on the
front of the sun-- some 1 million miles across from end to end.
Filaments are clouds of solar material suspended above the sun by
powerful magnetic forces. Though notoriously unstable, filaments can
last for days or even weeks.
A
dark snaking line in the upper right of these images on Sept. 30, 2014,
show a filament of solar material hovering above the sun's surface.
NASA's SDO captured the images in extreme UV light – different colors
represent different wavelengths of light and different temperatures of
solar material. Image Credit: NASA/SDO. View left image
NASA's
Solar Dynamics Observatory, or SDO, which watches the sun 24 hours a
day, has observed this gigantic filament for several days as it rotated
around with the sun. If straightened out, the filament would reach
almost across the whole sun, about 1 million miles or 100 times the size
of Earth.
SDO captured images of the filament in numerous wavelengths, each of
which helps highlight material of different temperatures on the sun. By
looking at any solar feature in different wavelengths and temperatures,
scientists can learn more about what causes such structures, as well as
what catalyzes their occasional giant eruptions out into space.
Look at the images to see how the filament appears in different
wavelengths. The brownish combination image was produced by blending two
wavelengths of extreme UV light with a wavelength of 193 and 335
Angstroms. The red image shows the 304 Angstrom wavelength of extreme UV
light.