To everyone’s surprise it has
been discovered that occasional flares are followed sometimes an hour and a
half later by a second event that is in the extreme ultraviolet with as much as
four times the original energy.
I suspect that we will also
observe a number of rarer features presently unknown with solar flares as we
continue to gather data during this particular sunspot maximum. No one is complaining about a lack of sun
spots any more.
Our ability to survey the solar
system is now increasing rapidly and our present limit is solely our
imagination easily overcome by simply getting out there.
The Secret Lives of Solar Flares
Sept. 19, 2011: One hundred and fifty two years ago, a man in England named
Richard Carrington discovered solar flares.
Sunspots sketched by R. Carrington on Sept. 1, 1859. © R.
Astronomical Society. [more]
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 fading away.
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. Researchers recently announced
that solar flares have been keeping a secret.
“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.”
Click to view a ScienceCast video about the late phase of solar flares.
[Youtube]
NASA’s Solar Dynamics Observatory (SDO), launched in February 2010,
made the finding: About 1 in 7 flares experience an
“aftershock.” About ninety minutes 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.”
What causes the late phase? Solar flares happen when the magnetic
fields of sunspots erupt—a process called “magnetic reconnection.” The
late phase is thought to result when some of the sunspot’s magnetic loops
re-form. A diagram prepared
by team member Rachel Hock of the University
of Colorado shows how it
works.
The extra energy from the late phase can have 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 nearly 24 hours a day, 7
days a week. With that kind of scrutiny, it’s tough to keep a
secret--even one as old as this.
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