IMAGE
Meetings and Workshops
Meetings and Workshops
Image of IMAGE in space

EUV Team Meeting

University of Arizona
Tucson, AZ
21-22 October 2003
 

Logistics

Logistical information for the meeting is provided at http://euv.lpl.arizona.edu/euv/2003meetings/.

For attendees staying at the Sheraton Four Points:

The distance from the Sheraton Four Points to the EUV and FUV meetings in the Gould-Simpson Building is about 1.6 km over flat terrain. For those who prefer not to walk or drive their own car, a van from the Lunar and Planetary Laboratory will make several trips from the Sheraton to the Gould-Simpson Building beginning at about 8:20 a.m. on Tuesday morning. It will also be available for the return trip after the meetings.

Walkers Caution! The EUV and FUV meetings are not in the Kuiper Space Sciences Building, which many of you may be familiar with as the home of most of LPL. To find the Gould-Simpson Building, please consult the section "EUV and FUV Meetings" at http://euv.lpl.arizona.edu/euv/2003meetings/ and the map that you will find there.

Agenda

Tuesday Morning, 21 October

Time Title Presenter
9:00 a.m. Meeting Logistics, This and That Sandel
9:10 a.m. EUV Status Sandel
9:20 a.m. EUV Analysis Details: Plate Scale, overlap changes, work toward automatic Earth centering Sandel
9:40 a.m. New and updated EUV software: euv_imtool enhancements, FITS extraction, catalog, recon Forrester
10:15 a.m. Break
10:45 a.m. New software Gurgiolo
11:20 a.m. Kilometric continuum-GEOTAIL, IMAGE RPI, IMAGE EUV Green
12:00 p.m. Lunch  

Tuesday Afternoon, 21 October, Joint FUV/EUV session

Time Title Presenter
1:00 p.m. Observation of sub-auroral protons flashes with FUV Hubert
1:30 p.m. Generation of sub-auroral proton arcs and the importance of hot-cold plasma interactions Fuselier
2:00 p.m. Sub-Corotation in the plasmasphere Burch
2:30 p.m. Properties of the Plasmasphere Sub-Corotation from IMAGE/EUV Ballester
3:00 p.m. Cookies  
3:30 p.m. Recent progress in EUV/ground-based comparisons Foster
4:00 p.m. Plasmasphere/ring current overlap Gurgiolo
4:30 p.m. Global plasmaspheric dynamics and L-shell dependent rotations from inverted data from IMAGE EUV Larsen

Wednesday Morning, 22 October

Time Title Presenter
9:00 a.m. Extracting edges from non-polar images Roelof
9:40 a.m. Prospects for determining the 3D He+ distribution from EUV images Herbert
10:20 a.m. Break  
10:40 a.m. Thoughts on the "W" notch events Gallagher
11:20 a.m. Practical Electric Field Extraction from EUV Images Goldstein
12:00 p.m. Lunch  

Wednesday Afternoon, 22 October, Joint with FUV?

Time Title Presenter
1:30 p.m. An attempt to determine the major contributions to the EUV-observed aurora. Joint with FUV? Gladstone

For questions about the meeting, contact Bill Sandel.

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Curators

Dr. E. V. Bell, II, ed.bell@nasa.gov, +1-301-286-1187
NSSDC, Mail Code 690.1, NASA Goddard Space Flight Center, Greenbelt, MD 20771
 
Dr. D. R. Williams, dave.williams@gsfc.nasa.gov, +1-301-286-1258
NSSDC, Mail Code 690.1, NASA Goddard Space Flight Center, Greenbelt, MD 20771
NASA Official: Dr. David R. Williams Rev. 1.1.1, 20 October 2003