From mkaiser@lepmlk.gsfc.nasa.gov Fri Apr 20 08:45:11 2001 Return-Path: Received: from wheelo.gsfc.nasa.gov (wheelo.gsfc.nasa.gov [128.183.254.141]) by sag.lmsal.com (8.11.0/8.11.0) with ESMTP id f3KFj4J07042 for ; Fri, 20 Apr 2001 08:45:04 -0700 (PDT) Received: from lepmlk.gsfc.nasa.gov (lepmlk.gsfc.nasa.gov [128.183.20.50]) by wheelo.gsfc.nasa.gov (8.9.3/8.9.3) with ESMTP id LAA05730; Fri, 20 Apr 2001 11:44:25 -0400 (EDT) Received: from lepmlk.gsfc.nasa.gov (lepmlk.gsfc.nasa.gov [128.183.20.50]) by lepmlk.gsfc.nasa.gov (8.9.3+Sun/8.9.1) with SMTP id LAA01521; Fri, 20 Apr 2001 11:42:10 -0400 (EDT) Message-Id: <200104201542.LAA01521@lepmlk.gsfc.nasa.gov> Date: Fri, 20 Apr 2001 11:42:10 -0400 (EDT) From: Mike Kaiser Reply-To: Mike Kaiser Subject: WAVES April 18 report To: reiner@urap.gsfc.nasa.gov, thompson@eitv3.nascom.nasa.gov, stcyr@cua.edu, bale@sunspot.ssl.berkeley.edu, ennio.sanchez@sri.com, robert.macdowall@gsfc.nasa.gov, mdryer@sec.noaa.gov, u2leb@lepvax.gsfc.nasa.gov, bougeret@obspm.fr, gopals@fugee.gsfc.nasa.gov, ipavich@umtof.umd.edu, nitta@lmsal.com, kaiser@lepmlk.gsfc.nasa.gov, xrdbb@lepvx3.gsfc.nasa.gov, golla@urap.gsfc.nasa.gov, kartalev@geospace4.imbm.bas.bg, bfleck@esa.nascom.nasa.gov, RWC.BOULDER@noaa.gov, space@afwa.af.mil, roger-r-anderson@uiowa.edu, u2dhf@lepdhf.gsfc.nasa.gov, zsmith@sec.noaa.gov, eort@sec.noaa.gov, nigel@ips.gov.au, bmurtagh@sec.noaa.gov, gfry@expi.com, ccwu@bxsvr2.bartol.udel.edu, gheckman@sec.noaa.gov, plunkett@kreutz.nascom.nasa.gov, hudson@isass0.solar.isas.ac.jp, ebend@netlabs.net, cbalch@sec.noaa.gov, nicola.fox@gsfc.nasa.gov, hilary.cane@utas.edu.au MIME-Version: 1.0 Content-Type: TEXT/plain; charset=us-ascii Content-MD5: Sg284by1ab8HTvWhzB6Zmg== X-Mailer: dtmail 1.3.0 @(#)CDE Version 1.3.5 SunOS 5.7 sun4u sparc Status: R WAVES detected a type II associated with the April 18 proton event. WAVES observed an intermittent type II from about 02:55 UT (10 MHz) to about 14:00 UT (100 kHz). This type II was preceded by the usual SA type IIIs between 02:15 and 02:45. Rough speed estimate with the usual assumptions would be about 950 km/sec or so. This is quite a bit higher than the 550 km/sec from Culgoora, although the early part of our event near the sun seems to fit their speed pretty well. It's the 100 kHz stuff that needs the high speed. Using our speed, the shock would arrive at 1 AU sometime after 23 UT on April 20. MLK