| Sunday,
November 2, 2003 |
| 7:00-8:30
pm |
Welcome
Reception/Registration (Canyon Room) |
|
|
| Monday,
November 3, 2003 |
| Notes:
|
1.
Canyon Room is downstairs, Catalina Room is upstairs; all talks in
Catalina Room.
2. Speakers only are listed here, co-authors given in abstracts.
3. Provided meals are: breakfast 3 days, lunch Monday, and banquet
Tuesday. |
|
|
| 7:00
am |
Breakfast
and Registration (Canyon Room) |
|
|
| 7:45
am |
Welcome/Announcements
(Catalina Room) |
|
|
| Particle
heating during reconnection |
|
|
| 8:00
am |
R.
Lin (Space Sciences Lab, U.C. Berkeley, USA)
RHESSI Observations of Magnetic Reconnection, Energy Release, and
Particle Acceleration in a Large Solar Flare |
| 8:30
am |
M.
Hoshino (University of Tokyo, Japan)
Plasma Heating and Acceleration in Relativistic Magnetic Reconnection
and Current Driven Instability |
| 9:00
am |
M.
Øieroset (Space Sciences Lab, U.C. Berkeley, USA)
Evidence for Electron Acceleration up to ~300 keV in the Magnetic
Reconnection Diffusion Region of the Earth's Magnetotail: Wind Observations |
|
|
| 9:30
am |
coffee |
|
|
| 10:00
am |
J.
Birn (Los Alamos National Lab, USA)
Particle Heating in the Dynamic Magnetotail |
| 10:30
AM |
Y.
Ono (University of Tokyo, Japan)
Current Sheet Dynamics TS-3/4 Reconnection / Merging Experiments
|
|
|
| 11:00
am |
Discussion
1 (30 minutes) |
|
|
| 11:30
am |
Lunch
(Canyon Room, 45 minutes) |
|
|
| 12:15
pm |
Go
to Island Plaza for Inland Tour boarding pass pick-up at 12:30 |
|
|
| 12:45
pm |
Inland
Tour (optional, 3 hours 45 minutes duration, return about 4:30pm) |
|
|
| Jets,
dynamo, and reconnection |
|
|
| 5:15
pm |
S.
Hirose (Johns Hopkins University, USA)
Numerical Examination of an Exact Solution for Incompressible Magnetic
Reconnection |
| 5:45
pm |
T.
Kudoh (University of Western Ontario, Canada)
Magnetically Driven Model of Astrophysical Jets: Theory and Numerical
Simulation |
|
|
| 6:15
pm |
dinner
break |
|
|
| 8:30
pm |
P.
Bellan (Caltech, USA)
Simulating Solar and Astrophysical Plasmas in Laboratory Experiments
and New Models Motivated by these Experiments |
| 9:00
pm |
H.
Li (Los Alamos National Lab, USA)
Extragalactic Magnetic Fields and Force-Free Reconnection |
|
|
| 9:30
pm |
Discussion
2 (30 minutes) |
