Mighty Streams of Plasma Flow under Solar Surface
News story originally written on September 3, 1997



Solar rotation at different depths (red being the fastest, blue the slowest)
Click on image for full size (96K JPEG)
Courtesy of NASA
With the help of the SOHO spacecraft, scientists have made an exciting discovery about the Sun. SOHO stands for Solar and Heliospheric Observatory.

The discovery is that there are streams of plasma flowing under the surface of the Sun. Plasma is really hot gas. These plasma streams are the smallest things found inside the Sun, but each stream is still big enough to hold two Earths!

These streams affect "weather" or activity. Activity on the Sun like solar flares affects the Earth. This activity can cause power outages and communications failures on Earth.

For the last year, the SOHO spacecraft has been a solar observatory. It is 930,000 miles away from the Earth and has 12 scientific instruments.

The SOHO mission homepage

Mighty Streams of Plasma Flow under Solar Surface
News story originally written on September 3, 1997



Solar rotation at different depths (red being the fastest, blue the slowest)
Click on image for full size (96K JPEG)
Courtesy of NASA
With the help of the SOHO (Solar and Heliospheric Observatory) spacecraft, scientists have made an exciting discovery about the Sun.

The discovery is that there are streams of plasma flowing beneath the surface of the Sun. Plasma is hot, electrically-charged gas. These plasma streams are the smallest things found inside the Sun, but each stream is still large enough to hold two Earths!

It is thought that these streams affect solar "weather" or activity. This new finding will help scientists to understand solar activity which directly affects the Earth. High solar activity can cause occasional power and communications disruptions on Earth.

For the last year, the SOHO spacecraft has been a solar observatory. It is 930,000 miles away from the Earth and has 12 scientific instruments. Scientists are excited about this recent discovery and look forward to future observations as the Sun enters its next active cycle around the year 2001.

The SOHO mission homepage

Mighty Streams of Plasma Flow under Solar Surface
News story originally written on September 3, 1997



Solar rotation at different depths (red being the fastest, blue the slowest)
Click on image for full size (96K JPEG)
Courtesy of NASA
With the help of the SOHO (Solar and Heliospheric Observatory) spacecraft, scientists at Standford University have made some exciting discoveries. The first discovery is that there are streams of plasma flowing beneath the surface of the Sun. "We have detected motion similar to the weather patterns in the Earth's atmosphere," said Dr. Jesper Schou of Stanford. "This flow is totally inside the Sun. It is completely unexpected, and cannot be seen at the surface."

These plasma streams are the smallest structures yet observed inside the Sun, but each stream is still large enough to engulf two Earths. It is thought that these streams may indeed affect solar "weather" or activity. These new findings will help scientists to understand increases in solar activity which directly affects the Earth causing occasional power and communications disruptions.

The second solar discovery is bands of gas similar to the Earth's trade winds. Standford scientists have found that there are gaseous bands located in both hemispheres that move faster than the material around them. These bands extend to a depth of at least 12,000 miles below the Sun's surface. These bands also have a relationship to sunspot formation as sunspots form at the edges of these zones.

For the last year, the SOHO spacecraft has acted as a solar observatory. It is 930,000 miles away from the Earth and has 12 scientific instruments. Scientists are excited about these recent discoveries and look forward to future observations as the Sun enters its next active cycle around the year 2001.

The SOHO mission homepage


Last modified prior to September, 2000 by the Windows Team

The source of this material is Windows to the Universe, at http://www.windows.ucar.edu/ at the University Corporation for Atmospheric Research (UCAR). © The Regents of the University of Michigan. Windows to the Universe® is a registered trademark of UCAR. All Rights Reserved. Site policies and disclaimer