EDI Prime Parameter Data
EDI data is available from the Cluster Active Archive
NOTES:
1. EDI processed data are obtained by combining multiple return-beams
within each analysis interval, using either the triangulation or
time-of-flight technique, to determine the drift velocity perpendicular to
B. The data files contain both the drift velocity, and associated (-VxB)
electric field, in inertial GSE coordinates (after subtracting the
spacecraft velocity). The ground analysis provides a statistical assessment
of the "quality" of each result, which we classify as "good", "caution", or
"bad". The PP data available here were processed using a single spin (4
second) analysis interval, and have been filtered to retain only "good"
results. The assignment of "good" is based on an automated algorithm, and
should not be taken as a guarantee of each point. In some instances
improved results can be obtained with manual adjustments to the filtering,
analysis intervals, or processing parameters. For assistance or with
questions about individual events, please contact the EDI team:
Goetz Paschmann, goetz.paschmann (at) mpe.mpg.de
Jack Quinn, jack.quinn(at)unh.edu
Last modified: Thu May 22 15:40:08 EDT 2008