Sun  ID: 12618

How Plasma Transports Energy

Observational proof of a 50-year-old theory has reshaped the basic understanding of a type of wave in space known as a kinetic Alfvén wave. Kinetic Alfvén waves have long been suspected to transport energy in plasmas, a fundamental state of matter composed of charged particles that exists throughout the universe. For the first time, scientists working with NASA’s Magnetospheric Multiscale (MMS) mission have been able to directly examine the microphysics of kinetic Alfvén waves in the Earth’s magnetosphere. As these waves move through a plasma, electrons traveling at the right speed get captured in weak spots of the wave’s magnetic field. Other electrons in the plasma traveling faster or slower than the wave end up passing energy back and forth as they try to keep up with it. This is similar to how a car’s cruise control works: If the car is going faster than the set limit, the car will lose energy to slow down and if the car is going slower than the limit, it will gain energy to speed up. By understanding the fundamental process that transports energy through a plasma, NASA can improve nuclear fusion technology and better understand how the solar wind - the constant flow of solar particles that bathes the entire solar system - is heated to extreme temperatures. Watch the video to learn more.

Source Material

Related Stories

For More Information

Story Credits

Lead Visualizers/Animators:
Tom Bridgman (Global Science and Technology, Inc.)
Brian Monroe (USRA)

Lead Producer:
Genna Duberstein (USRA)

Lead Scientist:
Daniel J. Gershman (University of Maryland College Park)

Lead Writers:
Mara Johnson-Groh (Wyle Information Systems)
Jordan Rice (Intern)

Please give credit for this item to:
NASA's Scientific Visualization Studio

Short URL to share this page:

SVS >> App
NASA Science >> Sun