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The Secret Lives of Solar Flares.
Brought to you by Science at NASA.
152 years ago, a man in England named Richard Carrington
discovered solar flares.
It happened at 11:18 AM on the cloudless morning of
Thursday, September 1st, 1859.
Just as usual on every sunny day, the 33-year-old solar
astronomer was busy in his private observatory, projecting
an image of the sun onto a screen and sketching what he saw.
On that particular morning, he traced the outlines of an
enormous group of sunspots.
Suddenly, before his eyes, two brilliant beads of white
light appeared over the sunspots; they were so bright he
could barely stand to look at the screen.
Carrington cried out, but by the time a witness arrived
minutes later, the first solar flare anyone had ever seen
was over.
It would not be the last.
Since then, astronomers have recorded thousands of strong
flares using instruments ranging from the simplest
telescopes in backyard observatories to the most complex
spectrometers on advanced spacecraft.
Possibly no other phenomenon in astronomy has been studied
as much.
After all that scrutiny, you might suppose that everything
about solar flares would be known.
Far from it.
Last week, researchers announced that solar flares have
been keeping a secret-and it's a big one.
"We've just learned that some flares are many times
stronger than previously thought," says University of
Colorado physicist Tom Woods who led the research team.
"Solar flares were already the biggest explosions in the
solar system and this discovery makes them even bigger."
NASA's Solar Dynamics Observatory, launched in February
2010, revealed the secret: About 1 in 7 flares experience a
sort of "aftershock."
Ninety minutes or so after the flare dies down, it springs
to life again, producing an extra surge of extreme
ultraviolet radiation.
"We call it the 'late phase flare,'" says Woods.
"The energy in the late phase can exceed the energy of the
primary flare by as much as a factor of four."
The extra energy has a big effect on Earth.
Extreme ultraviolet wavelengths are particularly good at
heating and ionizing Earth's upper atmosphere.
When our planet's atmosphere is heated by extreme UV
radiation, it puffs up, accelerating the decay of
low-orbiting satellites.
Furthermore, the ionizing action of extreme UV can bend
radio signals and disrupt the normal operation of GPS.
SDO was able to make the discovery because of its unique
ability to monitor the sun's extreme UV output in high
resolution 24 hours a day, 7 days a week.
With that kind of scrutiny, it's tough to keep a
secret, even one that's 152 years old.
To learn more secrets of astronomy, visit science.nasa.gov.