Subject: Re: Correction to Oct, 2001 Event for COSPAR Date: Tue, 10 Sep 2002 20:00:29 +0200 From: Ondrej Santolik To: Jolene Pickett CC: mparrot@cnrs-orleans.fr, zong@bu.edu, Mark.L.Adrian@msfc.nasa.gov, pdecreau@cnrs-orleans.fr, patrick.canu@cetp.ipsl.fr, amasson@so.estec.esa.nl, harri.laakso@esa.int, ".jolene pickett" , mohammed.boudjada@oeaw.ac.at, bell@nova.stanford.edu, fritz@bu-ast.bu.edu, nicole.cornilleau@cetp.ipsl.fr, Mats.Andre@irfu.se Dear Jolene, Sorry for a late reply, I've been moving to Orleans to work with Michel this week before the Cluster workshop. STAFF-SA data for the cases we have already discussed (July 9, 2001, Oct. 21, 2001, and Mar. 11, 2002) are at http://www-pw.physics.uiowa.edu/~os/staff_sa/data/ We have now processed the March 25, 2002 case and you can download the figures from ftp://canopus.cnrs-orleans.fr/pub/santolik/ The whistler-mode emissions between 1 and 4 kHz in your time interval propagate to the North, away from the equator, like chorus usually does. The wave normals seem to be inclined from the B0 direction by 20-60 degrees toward higher L shells. This could correspond to propagation effects, supposing a source region of quasiparallel waves close to the equator. Please let me know if you want any detailed figures showing the same time interval as on WBD, or a combined plot of both instruments. Best regards Ondrej