Now that we are able to look
closely, we are finding out just now active the sun can be. No one imagined this or that such an event
would go unnoticed on Earth but from our observation gear now in place.
The importance of this eruption
is not so much the event itself however unprecedented as the discovery of
direct linkage on a global basis for the large events. This completely resets our models and general
thinking.
I recall when we expected little
from the sun in new data. Now we are
looking at a variable star up close in 360 degrees and getting all the action
we could ever desire.
The miracle is how well shielded
we are and have been for billions of years.
Global Eruption Rocks the
Sun
Dec. 13, 2010: On August 1,
2010, an entire hemisphere of the sun erupted. Filaments of magnetism snapped
and exploded, shock waves raced across the stellar surface, billion-ton clouds
of hot gas billowed into space. Astronomers knew they had witnessed something
big.
It was so big, it may have shattered old ideas
about solar activity.
"The August 1st event really opened our
eyes," says Karel Schrijver of Lockheed Martin’s Solar and Astrophysics
Lab in Palo Alto ,
CA. "We see that solar storms can be global events, playing out on scales
we scarcely imagined before."
Click to play an extreme ultraviolet
movie of the August 1st global eruption. Different colors represent different
plasma temperatures in the range 1.0 to 2.2 million K. Credit: Solar Dynamics
Observatory.
For the past three months, Schrijver has been
working with fellow Lockheed-Martin solar physicist Alan Title to understand
what happened during the "Great Eruption." They had plenty of data:
The event was recorded in unprecedented detail by NASA's Solar Dynamics
Observatory and twin STEREO spacecraft. With several colleagues present to offer
commentary, they outlined their findings at a press conference today at the
American Geophysical Union meeting in San
Francisco .
Explosions on the sun are not localized or
isolated events, they announced. Instead, solar activity is interconnected by magnetism
over breathtaking distances. Solar flares, tsunamis, coronal mass
ejections--they can go off all at once, hundreds of thousands of miles apart,
in a dizzyingly-complex concert of mayhem.
"To predict eruptions we can no longer
focus on the magnetic fields of isolated active regions," says Title,
"we have to know the surface magnetic field of practically the entire sun."
This revelation increases the work load for
space weather forecasters, but it also increases the potential accuracy of
their forecasts.
"The whole-sun approach could lead to
breakthroughs in predicting solar activity," commented Rodney Viereck of
NOAA's Space Weather Prediction Center in Boulder, CO. "This in turn would
provide improved forecasts to our customers such as electric power grid
operators and commercial airlines, who could take action to protect their
systems and ensure the safety of passengers and crew."
In a paper they prepared for the Journal of
Geophysical Research (JGR), Schrijver and Title broke down the Great Eruption
into more than a dozen significant shock waves, flares, filament eruptions, and
CMEs spanning 180 degrees of solar longitude and 28 hours of time. At first it
seemed to be a cacophony of disorder until they plotted the events on a map of
the sun's magnetic field.
Title describes the Eureka ! moment: "We saw that all
the events of substantial coronal activity were connected by a wide-ranging
system of separatrices, separators, and quasi-separatrix layers." A
"separatrix" is a magnetic fault zone where small changes in
surrounding plasma currents can set off big electromagnetic storms.
Locations of key events are labeled in this
extreme ultraviolet image of the sun, obtained by the Solar Dynamics
Observatory during the Great Eruption of August 1st. White lines trace the
sun's magnetic field. Credit: K Schrijver & A. Title. [larger image]
Researchers have long suspected this kind of
magnetic connection was possible. "The notion of 'sympathetic' flares goes
back at least three quarters of a century," they wrote in their JGR paper.
Sometimes observers would see flares going off one after another--like
popcorn--but it was impossible to prove a link between them. Arguments in favor
of cause and effect were statistical and often full of doubt.
"For this kind of work, SDO and STEREO
are game-changers," says Lika Guhathakurta, NASA's Living with a Star
Program Scientist. "Together, the three spacecraft monitor 97% of the sun,
allowing researchers to see connections that they could only guess at in the
past."
To wit, barely two-thirds of the August event
was visible from Earth, yet all of it could be seen by the SDO-STEREO fleet.
Moreover, SDO's measurements of the sun's magnetic field revealed direct
connections between the various components of the Great Eruption—no statistics
required.
Much remains to be done. "We're still
sorting out cause and effect," says Schrijver. "Was the event one big
chain reaction, in which one eruption triggered another--bang, bang, bang--in
sequence? Or did everything go off together as a consequence of some greater
change in the sun's global magnetic field?"
Further analysis may yet reveal the underlying
trigger; for now, the team is still wrapping their minds around the global
character of solar activity. One commentator recalled the old adage of three
blind men describing an elephant--one by feeling the trunk, one by holding the
tail, and another by sniffing a toenail. Studying the sun one sunspot at a time
may be just as limiting.
"Not all eruptions are going to be
global," notes Guhathakurta. "But the global character of solar
activity can no longer be ignored."
As if the sun wasn't big enough already….
keeping an eye on the entire solar magnetic activity can help a lot.the proper magnetic mapping and constant data recording of the solar atmosphere is very important.the sun is too big to ignore the surface solar activities.
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