A Solar Prominence Eruption from SDO
Explanation:
One of the most spectacular solar sights is an erupting prominence.
In 2011, NASA's Sun-orbiting
Solar Dynamic Observatory spacecraft imaged an
impressively large prominence
erupting from the surface.
The dramatic explosion was captured in ultraviolet light in the
above time lapse video covering 90 minutes, where a
new frame was taken every 24 seconds.
The scale of the prominence is huge -- the entire
Earth would easily fit under the flowing
curtain of hot gas.
A
solar prominence is channeled and sometimes held above the
Sun's surface by the Sun's
magnetic field.
A quiescent
prominence typically lasts about a month, and may erupt in a
Coronal Mass Ejection (CME)
expelling hot gas into the
Solar System.
The energy mechanism that creates a
solar prominence is still a topic of
research.
As the Sun passes
Solar Maximum,
solar activity like
eruptive prominences
are expected to become less common over the next few years.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
