Killer electrons in space are now less mysterious

The Sun-Earth connection
26 July 2007

A rare, timely conjunction of ground-based instrumentation and a dozen satellites has helped scientists better understand how electrons in space can turn into ‘killers’. ESA’s Cluster constellation has contributed crucially to the finding.

‘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.

Earth’s magnetic field
Earth’s magnetic field

The results come from complementary studies performed by teams led by Jonathan Rae at the University of Alberta, Canada and Qiugang Zong from the University of Massachusetts, Lowell, USA.

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.

Alignment of satellites on 25 November 2001
Alignment of satellites on 25 November 2001

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.

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.

Map of simultaneous observations

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.

Influence of solar wind on Earth's magnetosphere

“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.

Notes for editors:

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 Journal of Geophysical Research.

‘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.

For more information:

I. J. Rae, Department of Physics, University of Alberta, Canada
Email: JRae @ phys.ualberta.ca

Q. Zong, Center for Atmospheric Research, University of Massachusetts Lowell, USA
Email: Qiugang_Zong @ uml.edu

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

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