Allthough the Sun has been awfully quiet for a very long time, the new STEREO twin satellittes caught a major flare in May. The flare resulted in an intens Auroraover the South pole, which was imaged by the astronauts onboard the ISS

Solar storms bombard Earth with a stream of electrons and other charged particles that interact with gases in the atmosphere to generate colorful aurora. A coronal mass ejection, a large solar storm, can expel a billion tons of matter at a million miles per hour or more. The strongest solar storms have the potential to interfere with communications, power grids, and satellites. Solar storms happen most frequently when the Sun is in the active phase of its 11-year cycle, called solar maximum.

Though the Sun was expected to be entering solar maximum in 2010, it had been unusually quiet for at least two years. Despite its relative lack of activity, the Sun released a series of four coronal mass ejections between May 22 and May 24, 2010. These images show one coronal mass ejection on May 23. A movie of all four ejections is available on the Solar and Heliospheric Observatory web site.

Thiis image is taken by the Solar Terrestrial Relations Observations (STEREO) Ahead spacecraft from 20:09:15 Universal Time (UT). STEREO Ahead acquired the lower image just over two hours later at 22:24:00 UT. In the top image, a bright mass of charged particles loops from the Sun’s atmosphere. Two hours later, the looped mass had expanded and was moving away from the Sun. The images show only the Sun’s corona, the outermost layer of the atmosphere. A dark disk covers the rest of the Sun, and a white circle represents the Sun’s surface.

When the charged particles from May’s coronal mass ejections reached Earth, they caused no damage.

Among the views of Earth afforded astronauts aboard the International Space Station (ISS), surely one of the most spectacular is of the aurora.

These ever-shifting displays of colored ribbons, curtains, rays, and spots are most visible near the North (aurora borealis) and South (aurora australis) Poles as charged particles (ions) streaming from the Sun (the solar wind) interact with Earth’s magnetic field.

Source: Earth Observatory