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|    BAMA    |    Science Research Echo    |    1,586 messages    |
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|    Message 45 of 1,586    |
|    Roger Nelson to All    |
|    Global Eruption Rocks the Sun    |
|    13 Dec 10 17:19:34    |
      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.               URL:               http://science.nasa.gov/media/medialibrary/2010/12/13/globaldisruption.mov               [JEEZ!]               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.       [...]       NASA's twin STEREO spacecraft surround the sun. [STEREO home page] "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."       [...]       An artist's concept of the Solar Dynamics Observatory. [SDO home page] 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..                       Author: Dr. Tony Phillips | Credit: Science@NASA               More Information       Solar Dynamics Observatory -- SDO home page               Solar Terrestrial Relations Observatory -- STEREO home page                       Regards,               Roger              --- D'Bridge 3.58        * Origin: NCS BBS (1:3828/7)    |
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