Subject: Re: palm springs From: Simon Walker Date: Wed, 23 Feb 2005 15:48:35 +0000 (GMT) To: pickett@uiowa.edu Received: from moon.its.uiowa.edu (moon.its.uiowa.edu [128.255.56.76]) by kochab.physics.uiowa.edu (8.11.7p1+Sun/8.11.7) with ESMTP id j1NFmoR26200 for ; Wed, 23 Feb 2005 09:48:51 -0600 (CST) Received: from mailhub1.shef.ac.uk (mailhub1.shef.ac.uk [143.167.1.9]) by moon.its.uiowa.edu (8.12.10/8.12.9/uiowa-3.6) with ESMTP id j1NFmjPK017150 for ; Wed, 23 Feb 2005 09:48:46 -0600 Received: from vulture.shef.ac.uk ([143.167.44.8]) by mailhub1.shef.ac.uk with esmtp (Exim 4.43) id 1D3ykf-0005e3-Fe for pickett@uiowa.edu; Wed, 23 Feb 2005 15:48:45 +0000 Received: from skua (skua [143.167.52.52]) by vulture.shef.ac.uk (8.11.1/8.11.1) with SMTP id j1NFmZI25633 for ; Wed, 23 Feb 2005 15:48:35 GMT Message-ID: <200502231548.j1NFmZI25633@vulture.shef.ac.uk> Reply-To: Simon Walker MIME-Version: 1.0 Content-Type: MULTIPART/mixed; BOUNDARY=Sute_of_Bloodhounds_537_000 X-Mailer: dtmail 1.3.0 @(#)CDE Version 1.4.8 SunOS 5.8 sun4u sparc X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.2.0, Antispam-Data: 2005.2.23.6 Content-Length: 761115 Hi Jolene, I haven't left yet! I know Sheffield appears to be the back of beyond, almost at the ends of the Earth but it doesn't take that long to go anywhere. It just feels like it does. I plan to make my way to Heathrow tomorrow afternoon weather permitting . Its currently snowing and we have almost half an inch in Sheffield. This is usually more than enough to bring all types of transport to a grinding halt. We fly on Friday morning. > Many thanks for the plots. I finally got a chance to look at them at > home last night. Yes, they will do, but if you haven't left yet, could > you answer a couple of questions. What mode was EFW in to > make these measurements (burst?, filter?) ? The data come from the internal burst memory available within EFW. This memory stores data when some trigger condition is satisfied. The data is unfiltered, and is sampled at 9000Hz. > Also, what is the > conclusion from the velocity plot? Is it the case that the average > velocity of the structures is about 1000 km/s, heading upstream, > primarily in the direction of the ion foreshock? If not, can you > please et me straight. It looks to me like these examples you > sent all have time durations around 1 millisecond. If I have more > questions, I can probably catch you at the conference. I agree with your conclusions about the velocity plot. These features appear to propagate away from the shock front in the upstream direction. Perhaps this is due to the events analysed being in the foot region of the shock ie infront of the ramp. It is also interesting that the velocity vector appears to be neither perp nor para to B (see attached figure) in the spin plane. The problem may be that B is sampled at 22.*** Hz, and so small scale structures wil probably not be seen. This could also do with more statistics. Looking forward to seeing you and the Sun (in that order). Simon