‘Killer’ electrons are highly energetic, negatively charged particles found in near-Earth space. They can critically, and even permanently, damage satellites in orbit, including telecommunication satellites, and pose a hazard to astronauts.

Several theories have been formulated in the past to explain the origin of killer electrons, and many uncoordinated observations have already been performed. Recently, scientists got a boost in their understanding of this hazardous phenomenon. This was possible thanks to a unique set of data, collected simultaneously, by a global armada of ground and space observatories during the recovery phase of a large geomagnetic storm.




In the aftermath of the storm, the CARISMA (Canadian Array for Realtime Investigations of Magnetic Activity) magnetometer chain observed a type of Ultra Low Frequency (ULF) electromagnetic wave, well-known for creating killer electrons. CARISMA observed the so-called ‘Pc5 waves’ continuously, for many hours, during the recovery phase of a large geomagnetic storm on 25 November 2001. In the meantime, they were also picked up by more than half a dozen scientific satellites located inside Earth’s magnetic environment, or magnetosphere, including NASA’s Polar mission.

Meanwhile, ESA’s four Cluster satellites were located at the boundary of Earth’s magnetosphere, called the magnetopause. They observed undulations, or disturbances of the magnetopause, at the same frequency as that of Pc5 waves observed from inside the magnetosphere.

This composite image shows a SOHO image of the Sun and an artist's impression of Earth's magnetosphere. Credits: Magnetosphere: NASA, the Sun: ESA/NASA SOHO

Taking into account data from all satellites, Earth-based radars and magnetometers, Rae's team were able to reveal the mechanism behind the scenario.

During this event, the velocity of solar wind - a continuous stream of solar particles impacting and shaping Earth’s magnetosphere – was measured at approximately 750 km/s, nearly twice its average speed. The impact of this fast flow of solar particles on Earth’s magnetosphere induced the undulations observed by Cluster.

In turn, these undulations drove compressional waves, which propagated inward from the magnetopause towards Earth. Close to the location of the Polar satellite, these compressional waves coupled with Earth’s magnetic field lines, making the field lines resonate at the frequency of Pc5 waves, which are able to create killer electrons.

CLICK ABOVE FOR FULL SIZE. The diagram shows magnetic field lines generated by Earth’s magnetic field. As shown in the picture, the axis of the magnetic field is tilted with respect to Earth’s axis of rotation by 11.5 degrees. Credits: SCI-FUN (P. Reid)

Data from Cluster also played a key role in the findings of the study by Zong's team. They focused on the aftermath of another geomagnetic storm, which occurred on 31 October 2003. They not only confirmed that Pc5 waves accelerate electrons, but they have also succeeded in quantifying – for the first time, in situ – the velocity reached by the accelerated electrons.

“Earth’s magnetosphere is a very large, complex and variable system. This makes the understanding of ULF waves, together with the mechanisms for the energy transfer from space to ground, a very difficult matter,” says Philippe Escoubet, ESA's Cluster and Double Star Project Scientist.

This picture is an artist's impression of the influence of solar wind on Earth's magnetosphere. It results in the creation of instabilities in the magnetic field due to interaction between two superimposed fluids of differing densities and velocities along the magnetopause (Kelvin-Helmholtz surface waves). These surface waves waves create ULF waves, which in turn generate killer electrons. ESA’s Cluster constellation is depicted flying across. Credits: University of Massachusetts Lowell (Q. Zong)

“These new results on ULF waves and killer electrons once again highlight the need for simultaneous observations from space and ground. Only with constant monitoring with ground-based instruments can we put data obtained in space into a global context,” he added.

The paper ‘Evolution and characteristics of global Pc5 ULF waves during a high solar wind speed interval’ by I. Rae, E. Donovan, I. Mann, F. Fenrich, C. Watt, D. Milling, M. Lester, B. Lavraud, J. Wild, H. Singer, H. Rème, and A. Balogh has been published on 15 December 2005 in the Geophysical Research Letters.

‘Ultralow frequency modulation of energetic particles in the dayside magnetosphere’ by Q. Zong, X. Zhou, X. Li, P. Song, S. Fu, D. Baker, Z. Pu, T. Fritz, P. Daly, A. Balogh, and H. Rème has been published on 29 June 2007 in the Geophysical Research Letters.