Cotton Candy Sun
This still combines all of STEREO's wavelengths into one picture. NASA's Solar TErrestrial RElations Observatory (STEREO) satellites have provided the first three-dimensional images of the sun.
Another still combining all wavelengths from NASA's STEREO satellite reveals the upper part of the sun and its activity. "With STEREO's 3-D imagery, we'll be able to discern where matter and energy flows in the solar atmosphere much more precisely than with the 2-D views available before. This will really help us understand the complex physics going on," said Russell Howard of the Naval Research Laboratory, Washington, the Principal Investigator for the SECCHI (Sun Earth Connection Coronal and Heliospheric Investigation) suite of telescopes on the spacecraft.
This 2-D false-color image shows the sun's atmosphere at 1.8 million degrees Fahrenheit (1 million degrees Celsius). By looking at different temperatures, scientists can focus on different features of the sun.
This 2-D false-color image shows the sun's atmosphere at 2.7 million degrees Fahrenheit (1.5 million degrees Celsius).
Hint of Red
NASA's Solar Dynamics Observatory (SDO) mission created this magical shot from pairs of high-resolution images of the sun taken about eight hours apart on Dec. 4, 2011. Using imaging software, the scientists turned the results into a 3-D sun. The sun appears rounded and the loops above active regions clearly stand out above the sun's surface (as long as you're wearing 3-D glasses).
This color-coded image combines observations made by NASA's Solar Dynamics Observatory in several extreme ultraviolet wavelengths, highlighting a bright X-class flare toward the upper left of the sun's disk on March 6, 2012.
This 2-D false-color image shows the sun's atmosphere at 4.5 million degrees Fahrenheit (2.5 million degrees Celsius).
Green Sun Series
By combining images taken almost simultaneously from the Ahead and Behind STEREO spacecraft, researchers have generated a 3-D sequence of four images (clockwise starting at the top left) that track an active solar region over about a one-week period (April 29 through May 5, 2007). The images were all taken in extreme ultraviolet light. Active regions, which are areas of intense magnetic activity, appear brighter in UV light. The region is seen moving from left to right as the Sun's rotation carries it along. Arcing loops above the active region reveal million-degree Celsius particles spinning along magnetic field lines.
This is the first complete image of the solar far side, the half of the sun invisible from Earth. Captured on June 1, 2011, the composite image was assembled from NASA's two Solar TErrestrial RElations Observatory (STEREO) spacecraft. STEREO-Ahead's data is shown on the left half of image and STEREO-Behind's data on the right.
Remind anyone of a favorite arcade game? The new moon passes over the sun in this Feb. 21 image taken by NASA's Solar Dynamics Observatory. The partial eclipse was visible only from space.
The next partial solar eclipse Earthlings will be able to see will occur May 20, with views visible from Asia, the Pacific and western North America.
The gigantic sunspot in the upper left of this image is about 50,000 miles (80,000 km) long and was observed on the sun by NASA's Solar Dynamics Observatory on Nov. 3, 2011.