From: IN%"kent.tobiska@jpl.nasa.gov" "W. Kent Tobiska" 3-AUG-1999 22:54:42.95 To: IN%"Duane.L.Bindschadler@jpl.nasa.gov" "Duane Bindschadler" CC: IN%"kent.tobiska@jpl.nasa.gov", IN%"hendrix@pisces.colorado.edu" "Amanda Hendrix", IN%"stewart@pisces.colorado.edu" "Ian A.F. Stewart", IN%"Jim.Adams@lasp.colorado.edu" "Jim Adams", IN%"jajello@jpluvs.jpl.nasa.gov" "Joe Ajello" Subj: UVS/EUV C22 Science presentation Return-path: Received: from eis-msg-014.jpl.nasa.gov by pisces.colorado.edu (PMDF V4.2-13 #26137) id <01JECIVRLEPC9D4BTC@pisces.colorado.edu>; Tue, 3 Aug 1999 22:54:20 GMT Received: from [137.78.240.26] ([137.78.240.26]) by eis-msg-014.jpl.nasa.gov (8.9.3/8.9.3) with ESMTP id PAA02644; Tue, 3 Aug 1999 15:54:19 -0700 (PDT) Date: Tue, 03 Aug 1999 15:56:23 -0700 From: "W. Kent Tobiska" Subject: UVS/EUV C22 Science presentation In-reply-to: To: Duane Bindschadler Cc: kent.tobiska@jpl.nasa.gov, Amanda Hendrix , "Ian A.F. Stewart" , Jim Adams , Joe Ajello Message-id: MIME-version: 1.0 Content-type: text/plain; charset="us-ascii" Content-transfer-encoding: 7BIT X-Sender: ktobiska@pop.jpl.nasa.gov 22IUECLPSE01 Io aurora discovery observation in H I, O I, and H2 emissions. 22JULTN27902, 22JULTN29702, 22JUNEB28202, 22JUNEB29702, 22JUNEB31202, 22JUNEB32702, 22JUHTS26002, 22JUPOL29502, 22JUNOR29702 Ride-along with the SSI feature track observations to study stratospheric aerosols in the MUV. 22JUBRITSD01-08 Study acetylene and ammonia at several Jupiter latitudes and emission angles to understand minor species chemistry related to dynamics. 22JUAURORA01 Jupiter aurora observations of Lyman-alpha and H2 emissions near the 80 (S) longitude. We are studying the long-term magnetosphere and Jovian upper atmosphere interaction. This is a realtime observation for 1.5 hours using F/G full-scans. 22GUAURORA01 Ganymede aurora discovery observation in H I, and O I emissions. 22TV22NANS01, 22TU22NANS01-02 EUV/UVS map of Io torus noon ansa during the C22 outbound to determine morphological changes in torus over the timescale of several years and to look at dusk torus sectors. EUV emission lines: S++ 685, S+ 765, O+ 834; UVS emission lines:H 1215, S+ 1259, S+ 4070. ************************** W. Kent Tobiska FDC/JPL, MS 264-580 4800 Oak Grove Dr. Pasadena, CA 91109 (818) 393-7742 (phone) (818) 393-4530 (fax) kent.tobiska@jpl.nasa.gov http://www.spacenvironment.net **************************