Jupiter study points to better satellite protection

Scientists analysing the effects of radio waves on electrons in Jupiter’s magnetic field believe their work overturns a theory that has held sway for more than a generation and could be used to protect Earth-orbiting satellites from the devastating effects of radiation.

Using data collected at Jupiter by the Galileo spacecraft, Dr Richard Horne of British Antarctic Survey (BAS) and colleagues from the University of California, Los Angeles, and the University of Iowa found that a special type of very low frequency radio wave is strong enough to accelerate electrons up to very high energies inside Jupiter’s magnetic field. Their work has been published in Nature Physics.

Horne said: “We’ve shown before that very low frequency radio waves can accelerate electrons in the Earth’s magnetic field, but we have now shown that exactly the same theory works on Jupiter, where the magnetic field is 20,000 times stronger than the Earth’s and the composition of the atmosphere is very different. This is the ultimate test of our theory.

“On Jupiter, the waves are powered by energy from volcanoes on the moon Io, combined with the planet’s rapid rotation once every ten hours. Volcanic gasses are ionised and flung out away from the planet by centrifugal force. This material is replaced by an inward flow of particles that excite the waves that in turn accelerate the electrons.”

Understanding how electrons are accelerated will help scientists make better predictions of when satellites are at risk of damage by high-energy charged particles. These particles encircle the Earth in the Van Allen radiation belts and can damage satellites by causing malfunctions and degrading electronic components. However, the number of particles in the radiation belts can change dramatically within a few minutes, which is why more accurate forecasting is needed.

The discovery also has other scientific implications for Jupiter it overturns a theory that has held sway for more than 30 years. Horne explained: “For more than 30 years it was thought that the electrons are accelerated as a result of transport towards Jupiter, but now we show that gyro-resonant wave acceleration is a very important step that acts in concert. Once the electrons are accelerated, they are transported closer to the planet and emit intense synchrotron radiation out into interplanetary space. Our theory provides the missing step to explain this high intensity radiation from Jupiter, which was first detected on Earth more than 50 years ago.”

The volcanoes on Io contribute to the intense bursts of radiation encountered in Jupiter’s orbit

Recent articles

Info Message

Our sites use cookies to support some functionality, and to collect anonymous user data.

Learn more about IET cookies and how to control them

Close