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A closer look at ‘space weather’ Tracking the storms of the sun Satellite traces solar wind's source | |||
| THE EXPLOSIONS, called coronal mass ejections, occur several times a day, packing the power of billion-megaton nuclear blasts. Such storms send out a hail of electrically charged particles at a million miles an hour and if the blast happens to be pointed in Earths direction, it can affect radio communications, electrical power systems and satellites orbiting Earth. This event, although not common, is a disaster ... a very expensive event for the folks who rely on these systems, said Richard Canfield, a physicist at Montana State University at Bozeman. Scientists can spot a hazardous coronal mass ejection as it occurs, providing about four days of lead time to prepare for the storm. But Canfield said he and his colleagues have detected telltale warning signs that herald a coronal mass ejection two or three days before it even happens which could give power companies and satellite operators extra time to cover their assets. We have here a tool that we expect would be very useful for predicting conditions in space weather, he told reporters Tuesday at a NASA news briefing. SOLAR SLEUTHS The discovery is the subject of a paper to be published in the March 15 issue of Geophysical Research Letters. Analyzing two years worth of X-ray images from the Japanese-American Yohkoh satellite, Canfield and his colleagues found a link between S-shaped structures of brightly glowing gas on the suns surface and the rise of a coronal mass eruption. About two-thirds of the suns big eruptions develop from such structures, known as sigmoids, said Alphonse Sterling, a solar physicist at Computational Physics Inc. in Virginia. | |||||||||||||||||||||||||||
| Scientists believe the S-shaped structure is actually the signature of a twisted magnetic field on the suns surface. The magnetic field is what the plasma (superheated gas) is hanging on, explained Cambridge University researcher Sarah Gibson. She and her colleagues surmise that the twists build up tension like a twisted rubber band magnetic flux that is released in the explosive eruptions. Canfield said there was also a statistical correlation between the eruptions and sunspots, those relatively cool, dark areas that mottle the suns bright disk. If the S-shaped pattern is spotted in an area that has large sunspots, the sigmoid is virtually certain to erupt as it passes across the disk, he said. WHAT IT ALL MEANS The new findings are scientifically significant because they help flesh out theories on how the sun works and how the superstorms are created, experts said. The idea that twisted structures should erupt is not a new idea. This just brings a lot of specificity to that question, Canfield said. The findings also could lead the way to better forecasting of space weather, the scientists said. As it happens, the sun is headed toward the peak of an 11-year cycle of activity next year. During the last solar maximum, in 1989, a coronal mass ejection knocked out power to a wide area of Quebec for nine hours, noted George Withbroe, science director for NASAs Sun-Earth Connection research theme. He also referred to last years failure of the Galaxy 4 satellite, which led to widespread communications outages. | |||||||||||||||||||||||||||
With an extra couple of days of warning about solar storms, power companies could take further steps to protect transformers, and satellite operators could have more time to soften the brunt of the storm. However, Canfield said much more work needed to be done to turn sigmoid-spotting into a more precise predictive tool for coronal mass ejections. We need to get past simple classifications such as, Is it sigmoidal or not, is the sunspot big or small, and get to quantitative measurements that answer how twisted are the magnetic fields, how big is the spot, Canfield said. As well, we want to know in which direction the CME is going to go and how many regions are likely to erupt. NASA is planning a mission that will make three-dimensional images of coronal mass ejections and the structures around them called the Solar Terrestrial Relations Observatory, or STEREO to answer these questions, he said. Ultimately, Canfield said, the National Oceanic and Atmospheric Administration may be able to include warnings of coronal mass ejections in its space weather forecasts, in the same way that meteorologists make long-range forecasts on Earth. NOAA is building a Solar X-Ray Imager similar to that on Yohkoh that is scheduled for launch next year, he noted. | ||||||||||||||||||||||||||||
The Yohkoh Archive NOAA: Space Environment Center | |||
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