Filaments are ropes of solar material and magnetic fields, arcing up from the visible surface of the sun. When they erupt, they can produce solar flares and CMEs.
When a solar filament is viewed on the limb of the sun, it’s called a prominence.
Prominences (filaments) are anchored to the sun’s surface in its photosphere. They extend outward into the sun’s hot outer atmosphere, called the corona.
A filament or prominence forms over timescales of about a day. Stable prominences may persist in the corona for several months, looping hundreds of thousands of miles into space.
These structures can often be seen as red or pink features during a total solar eclipse.
Bottom line: Solar filaments (aka prominences, when viewed on the limb of the sun) are large, bright arcs of solar material and magnetic fields.
C. Alex Young is a solar astrophysicist studying the Sun and space weather. Alex is passionate about sharing science with diverse audiences. This led him to start The Sun Today with his designer wife, Linda. First through Facebook and Twitter then adding an extensive website thesuntoday.org, the two work together to engage the public about the Sun and its role in our solar system. Alex led national engagement efforts for the 2017 total solar eclipse. He is the Associate Director for Science in the Heliophysics Science Division at NASA Goddard Space Flight Center.
Like what you read? Subscribe and receive daily news delivered to your inbox.
Thank you! Your submission has been received!
Oops! Something went wrong while submitting the form.