Annales Geophysicae, 24, 275–289, 2006
SRef-ID: 1432-0576/ag/2006-24-275
© European Geosciences Union 2006
Annales
Geophysicae
Electric field measurements on Cluster: comparing the
double-probe and electron drift techniques
A. I. Eriksson1, M. André1, B. Klecker2, H. Laakso3, P.-A. Lindqvist4, F. Mozer5, G. Paschmann2,6, A. Pedersen7,
J. Quinn8, R. Torbert8, K. Torkar9, and H. Vaith2,8
1Swedish Institute of Space Physics, Uppsala, Sweden
2Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany
3Solar System Division, ESA/ESTEC, Noordwijk, Netherlands
4Alfvén laboratory, Royal Institute of Technology, Stockholm, Sweden
5Space Sciences Laboratory, University of California, Berkeley, CA, USA
6International Space Science Institute, Bern, Switzerland
7Department of Physics, Oslo University, Norway
8Space Science Center, University of New Hampshire, Durham, NH, USA
9Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Received: 16 June 2004 – Revised: 29 November 2005 – Accepted: 14 December 2005 – Published: 7 March 2006
Abstract. The four Cluster satellites each carry two instru-
ments designed for measuring the electric field: a double-
probe instrument (EFW) and an electron drift instrument
(EDI). We compare data from the two instruments in a rep-
resentative sample of plasma regions. The complementary
merits and weaknesses of the two techniques are illustrated.
EDI operations are confined to regions of magnetic fields
above 30 nT and where wave activity and keV electron fluxes
are not too high, while EFW can provide data everywhere,
and can go far higher in sampling frequency than EDI. On
the other hand, the EDI technique is immune to variations
in the low energy plasma, while EFW sometimes detects
significant nongeophysical electric fields, particularly in re-
gions with drifting plasma, with ion energy (in eV) below the
spacecraft potential (in volts). We show that the polar cap
is a particularly intricate region for the double-probe tech-
nique, where large nongeophysical fields