Magnetic environment at Earth and Jupiter

Observing Jupiter to understand Earth

5 December 2008

Magnetic substorms on Earth disrupt orbiting satellites, including telecommunication satellites and global positioning systems. This mysterious phenomenon has been studied with ESA’s Cluster satellites, comparing it with magnetic substorms on the giant planet Jupiter for a better understanding.

How the magnetosphere gets stormy

Planets such as Mercury, Earth or Jupiter that have their own magnetic field are protected by the magnetic bubble that it generates.

During a magnetic substorm on Earth, particles located tens of thousands kilometres on the nightside are energised and hurled earthward within a few minutes. This creates colourful aurorae and excites the near-Earth environment, disrupting communications between Earth and orbiting satellites and affecting global positioning systems. Despite decades of space-based research, several aspects of this phenomenon remain unknown.

One such unknown aspect is the mechanism that triggers these storms: it is not clear whether the storms are caused by processes internal to the magnetosphere or by other external processes (solar origin).

Dr Elena Kronberg and colleagues at the Max Planck institute for Solar System Research, Germany, decided to look away from Earth, to other planets, to see if they could learn something new.

The Jupiter connection

On Earth, a periodic substorm shows a gradual decrease followed by a rapid increase in the amount of particles that are hurled earthward. One such cycle takes 2-3 hours. At Jupiter, the same cycle takes 2-3 days. This duration is longer partly because of Jupiter’s stronger magnetic field and larger magnetosphere. The jovian magnetic field is so large that Jupiter’s magnetosphere envelopes the planet’s galilean moons: Io, Europa, Ganymede and Calisto.

After detailed analyses of data from several missions, Dr Kronberg said, “We’ve found that at Earth and Jupiter, the magnetic field undergoes the same three steps during a substorm: growth, expansion and recovery.”

Kronberg and colleagues studied data from NASA’s Galileo spacecraft. In 2007, they reported that periodic substorms at Jupiter were connected to the constant release of matter by the jovian satellite Io, which lies inside the jovian magnetosphere. This release of matter forms part of the mechanism that triggers the substorm. This means that the driver of this phenomenon is internal to the jovian magnetosphere.

Extrapolating this mechanism to the terrestrial magnetosphere, Kronberg and colleagues propose that under certain conditions, periodic magnetospheric substorms at Earth may be driven internally by plasma eroded from the plasmasphere, a region of Earth’s magnetosphere. This feeds the magnetosphere, providing the matter required to trigger a substorm.

"With Cluster, we’ve gained a better understanding of the processes taking place inside Earth’s magnetosphere; this has enhanced our understanding of how our Solar System works. And now we’re delighted to learn more from gigantic Jupiter itself.” remarked Philippe Escoubet, ESA’s Cluster Project Scientist.

Notes for editors:

The results appear in ‘Comparison of periodic substorms at Jupiter and Earth’ by E. Kronberg, J. Woch, N. Krupp, A. Lagg, P. Daly, and A. Korth published in the Journal of Geophysical Research, 12 April 2008.

For more information:

Elena Kronberg, Max Planck Institute for Solar System Research, Germany
Email: Kronberg @ mps.mpg.de

Philippe Escoubet, ESA Cluster Project Scientist
Email : Philippe.Escoubet @ esa.int

Arnaud Masson, ESA Cluster Scientist
Email: Arnaud.Masson @ esa.int

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