Text Size
NASA’s STEREO Spacecraft Reveals the Anatomy of Solar Storms
April 14, 2009

Additional imagery and background information for this story can be found here.


What if solar physicists could predict sun storms with the same accuracy and efficiency that meteorologists predict hurricanes?

In much the same way that satellites allow forecasters to see the inner workings and development of a hurricane from its origins until the moment it reaches shore, NASA’s STEREO spacecraft are now capturing images of solar storms and making real-time measurements of their magnetic fields from the moment they lift off the sun until the moment their pressure waves reach Earth's shores.

Eruptions from the sun’s outer atmosphere, or corona, can wreak havoc on earthly technology. These solar hurricanes, known as coronal mass ejections (CMEs), spew billions of tons of plasma into space at thousands of miles per hour and carry some of the sun’s magnetic field with it.

These solar storm clouds create a shock wave and a large, moving disturbance in the solar system. The shock can accelerate some of the particles in space to high energies, a form of "solar cosmic rays" that can be hazardous to spacecraft and astronauts. The CME material, which arrives days later, can disrupt Earth’s magnetic field, or magnetosphere, and upper atmosphere.

Observations from NASA’s twin Solar Terrestrial Relations Observatory (STEREO) spacecraft have allowed scientists to accurately measure for the first time the speed, trajectory, and three-dimensional shape of solar storms.

STEREO consists of two nearly identical observatories that make simultaneous observations of CMEs from two different vantage points. One observatory 'leads' Earth in its orbit around the sun, while the other observatory 'trails' the planet. STEREO’s two vantage points provide a unique view of the anatomy of a solar storm as it evolves and travels toward Earth. Once the CME arrives at the orbit of Earth, sensors on the satellites take in situ measurements of the solar storm cloud, providing a "ground truth" between what was seen at a distance and what is real inside the CME.

[image-69]The combination is providing solar physicists with the most complete understanding to date of the inner workings of these storms. It also represents a big step toward predicting when and how the impact will be felt at Earth. The separation angle between the satellites affords researchers to track a CME in three dimensions, something they have done several times in the past few years as they have learned to use this new space weather tool.

"We can now see a CME from the time it leaves the solar surface until it reaches Earth, and we can reconstruct the event in 3D directly from the images," said Angelos Vourlidas, a solar physicist at the Naval Research Laboratory, Washington, and project scientist for the Sun Earth Connection Coronal and Heliospheric Investigation aboard STEREO.

"The in situ measurements from STEREO and other near-Earth spacecraft link the physical properties of the escaping CME to the remote images," said Antoinette "Toni" Galvin, a solar physicist at the University of New Hampshire, and the principal investigator on STEREO’s Plasma and Suprathermal Ion Composition (PLASTIC) instrument. "This helps us to understand how the internal structure of the CME was formed and to better predict its impact on Earth."

Until now, CMEs could be imaged near the sun but the next measurements had to wait until the CME cloud arrived at Earth three to seven days later. STEREO’s real-time images and measurements give scientists a slew of information—speed, direction, and velocity—of a CME days sooner than with previous methods. As a result, more time is available for power companies and satellite operators to prepare for potentially damaging solar storms.

Much like a hurricane’s destructive force depends on its direction, size, and speed, the seriousness of a CME’s effects depends on its size and speed, as well as whether it makes a direct or oblique hit across Earth’s orbit.

CMEs disturb the space dominated by Earth's magnetic field. Disruptions to the magnetosphere can trigger the brightly colored, dancing lights known as auroras, or Northern and Southern Lights. While these displays are harmless, they indicate that Earth’s upper atmosphere and ionosphere are in turmoil.

Sun storms can interfere with communications between ground stations and satellites, airplane pilots, and astronauts. Radio noise from a storm can also disrupt cell phone service. Disturbances in the ionosphere caused by CMEs can distort the accuracy of Global Positioning System (GPS) navigation and, in extreme cases, induce stray electrical currents in long cables and power transformers on the ground.

The twin STEREO spacecraft were launched October 25, 2006, into Earth’s orbit around the sun. The mission is the third in NASA’s Solar Terrestrial Probes (STP) program.

NASA’s STEREO Spacecraft Reveals the Anatomy of Solar Storms: Briefing Materials

For more information about NASA’s STEREO mission, visit:

Laura Layton
Heliophysics News Team

Youtube Override: 
Angelos Vourlidas, SECCHI Project Scientist, talks about coronal mass ejections- explosions of the sun's atmosphere that propagate in space in the form of a cloud, and how the STEREO satellites are helping scientists reconstruct a three-dimensional view of their structures.
Image Credit: 
NASA's Goddard Spaceflight Center
Image Token: 
Image from animation depicting a coronal mass ejection (CME) as it erupts from the sun and speeds toward Earth.
This artist’s animation depicts STEREO’s COR1 imager capturing a coronal mass ejection (CME) as it erupts from the sun and speeds toward Earth.
Image Credit: 
NASA's Goddard Spaceflight Center/Walt Feimer
Image Token: 
Image Token: 
Page Last Updated: October 29th, 2014
Page Editor: Holly Zell