Solar Storm Warning!
"The halo CME was magnificent," says Gary Heckman, a space weather forecaster at the NOAA Space Environment Center. "Based on [the characteristics of the eruption], this looks like a sure bet to produce a geomagnetic storm."
The velocity of the ejected material was at least 908 km/s, says Dr. Simon Plunkett, an operations scientist with the SOHO coronagraph team at the Naval Research Laboratory and the Goddard Space Flight Center. "The CME should reach Earth in a little less than 48 hours. This would put its arrival around midday on Thursday, June 8."
Above: This frame from a
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They may sound menacing, but CMEs pose little danger to people on Earth. Our planet's magnetic field serves as an effective shield against solar wind storms. The same familiar force that causes compass needles on Earth to point north also extends far into space. When a CME hits the magnetosphere -- the region around Earth controlled by its magnetic field -- most of the incoming material is deflected away from our planet.
A Double Whammy
The June 6, 2000, coronal mass ejection was accompanied by two of the most intense solar flares since a brilliant eruption in February 2000.
"CMEs can occur without a flare," says Dr. David Hathaway, a solar physicist at the Marshall Space Flight Center, "but today is the more typical case where a flare is also part of the eruption.
"Solar flares and CMEs occur whenever there's a rapid, large-scale change in the Sun's magnetic field. The solar active region that produced the eruptions [on June 6] had a complicated magnetic configuration - oppositely directed magnetic fields were seen right next to each other."
Does this spate of solar activity means that Solar Maximum has finally arrived?
"This is an indication that solar maximum is upon us," says Hathaway. There is a common misconception that "Solar Max" is a single episode of high activity. Not so, Hathaway cautions. The solar maximum will last over an extended period of time, perhaps as long as two years interspersed with many powerful solar flares and CMEs.
|Parents and Educators: Please visit Thursday's Classroom for lesson plans and activities related to this story.|
Waiting and Watching
When the CME arrives, scientists aren't sure how big the geomagnetic storm will be.
"To get an intense geomagnetic storm from a CME we believe that two things must happen," says Dr. James Spann of the Marshall Space Flight Center, a co-investigator on an ultraviolet imaging camera in orbit aboard NASA's aurora-monitoring Polar satellite. "First, the disturbance must encounter the Earth's magnetic field directly, as opposed to a glancing blow. Second, the magnetosphere must already have stored energy, ready to be released in the form of aurora. If either of these two conditions fail, we're not likely to have an intense auroral display."
While no one is certain what will happen on the night of June 8, this is a rare opportunity to anticipate an auroral storm with two full days of advance warning. There's plenty of time to set up your camera and prepare late-night observing snacks. You may need a cup of coffee, because the best time to spot aurora borealis is usually during the hours around local midnight (in this case, around the 12 o'clock boundary between June 8 and 9). The Moon will be in a waxing quarter phase, sinking below the horizon at approximately 1:30 a.m. local time on June 9. That will afford dark skies between moonset and dawn for rural observers at mid-latitudes. Unfortunately for sky watchers at higher latitudes (where aurora sightings are usually best), the extended hours of twilight just two weeks before the summer solstice may obscure all but the most intense Northern Lights.
The Science@NASA April 6th, 2000, aurora gallery features a selection of photos with camera settings suitable for recording aurora borealis. More observing tips are available at Jan Curtis's web site "Home of the Northern Lights."
The View from Space
A fleet of NASA and NOAA satellites will be monitoring events in space when the CME disturbance arrives tomorrow. These include Polar, GEOTAIL, ACE, POES and others.
Researchers say that the timing of this event couldn't be better for NASA's newest space mission -- the Imager for Magnetopause to Aurora Global Exploration (IMAGE) -- a unique satellite dedicated to the study of space storms. IMAGE's 'first light' pictures of electrified gas in Earth's magnetosphere were released just this week.
Right: This sequence of pictures captured by the Ultraviolet Imager on NASA's Earth-orbiting Polar satellite shows an auroral storm over northern Asia on February 24, 2000. Because it records ultraviolet light, Polar's UV camera can see aurora from space on both the day and night sides of Earth. Polar is one of several missions operating as part of the International Solar Terrestrial Physics (ISTP) program. ISTP and IMAGE complement and support one another.
"Before IMAGE, if we wanted to understand what happened during a storm like the one that's coming, we had to combine thousands of point-by-point measurements taken by different satellites during many distinct storms," continued Gallagher. "No single satellite had a continuous, global view of all the action.
"It would be like trying to understand the rules of major league baseball if you were only allowed to watch a few random moments of different games while wearing blinders that only let you see a little bit of the field at once -- like the first base line or right field -- but nothing else. If you watched several different baseball fields in this way over many years, you might eventually start to put together what baseball is all about, but it would be very difficult. Now imagine what you can learn about the game if you were suddenly given sight and could see the whole field at once throughout every game.
"That's how it is with IMAGE and the magnetosphere. We can see the whole thing at once for the first time. I hate to take advantage of this comparison, but with IMAGE it's a whole new ball game!"
Stay tuned to Science@NASA for news and updates about the coming geomagnetic disturbance.
Below: Solar Flares are classified by their x-ray flux in the 1.0 - 8.0 Angstrom band as measured by the NOAA GOES-8 satellite. On June 6, 2000, two solar flares from active region 9026 registered as powerful X-class eruptions.
SOHO is a cooperative project between the European Space Agency (ESA) and NASA. The spacecraft was built in Europe for ESA and equipped with instruments by teams of scientists in Europe and the USA.
Southwest Research Institute manages the IMAGE project and leads the IMAGE science investigation. The IMAGE Principal Investigator is James L. Burch.Web Links
NOAA Space Environment Center -official forecaster of space weather events
SpaceWeather.com -daily updates and news about solar flares, coronal mass ejections and geomagnetic activity
More about the "magnetotail" and what causes aurora - from the NASA/Goddard Space Flight center
All about aurora - from the University of Alaska Geophysical Institute
Aurora FAQ - from the University of Alaska Geophysical Institute
Thursday's Classroom -- lesson plans and educational activities about space weather. - from NASA/GSFC
IMAGE home page - from the Southwest Research Institute
IMAGE home page - from NASA/GSFC
Science@NASA stories about IMAGE:
Innovative Space Weather Mission Nears Launch -- Feb. 24, 2000
The RADAR Cop in Space -- March 24, 2000
Space Weather Satellite Blasts Off -- March 27, 2000