filament (on the Sun)
A strand of relatively cool gas suspended by magnetic
fields over the solar photosphere
so that it appears as a dark line over the Sun's disk. A filament on the
limb of the Sun seen in emission against the
dark sky is called a prominence. Filaments
often mark areas of magnetic shearing and can be seen only in the centers
of strong spectral lines, such as H-alpha
or the H and K lines of calcium.
A filament channel is a broad pattern of fibrils
in the chromosphere, marking where
a filament may soon form or where a filament recently disappeared.
Related category
SOLAR
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