First Announcement
The Third Hinode Science Meeting
1-4 December 2009
Hitotsubashi Memorial Hall, Tokyo
Scientific Rationale
The Sun is the nearest star, and detailed knowledge on the Sun and
the interplanetary space is a key to understanding of the stars and
astrophysical plasmas. Solar and heliospheric physics has been
experiencing spectacular advances recently, and new views on the
Sun and the interplanetary space are emerging.
The major research targets of solar/stellar physics include the
generation mechanism of magnetic fields (the dynamo mechanism),
their manifestations on the one hand as the heating of the upper
atmosphere and the generation of outflows (winds), and on the other
hand as violent energy release of magnetic energy in the form of
flare explosions. The disturbances from the Sun affect the environment
of the earth (the space weather), and long-term variation of solar
radiation may influence the climate of the earth.
The researches into the Sun's magnetic fields and their surface
and interplanetary manifestations have been conducted by combining
space missions, ground-based observations, theoretical studies and
numerical simulations. The new data from space missions Hinode and
STEREO, plus the upcoming SDO (Solar Dynamics Observatory) mission
will mark the beginning of a new era in solar physics research.
The year 2009 is timely after three years of operation of both
the Hinode and STEREO missions.
The ground-based solar telescopes are evolving into a new phase
with one meter or bigger aperture and the state-of-the-art adaptive
optics system to fully utilize their large aperture. The advances
in computer technology have made it possible to simulate realistic
plasma dynamics and radiation processes in the solar atmosphere in
the computers. The combination of observational data and computer
simulation results is a powerful tool for the understanding
of basic physical processes in solar and astrophysical plasmas,
and will even be more so in the future.
This is the third Hinode symposium following the Hinode-1 in Dublin
(2007) and Hinode-2 in Boulder (2008). The symposium is not restricted
to the Hinode-related researches but
will include the recent results from other space missions,
ground-based instruments, and theoretical researches. Prospects of the
future missions and ground-based instrumentation will also be discussed.
Venue
The conference venue, Hitotsubashi Memorial Hall,
is located within National Center of Sciences,
of which another tenant is National Institute of Informatics
(
http://www.nii.ac.jp/introduce/access1.shtml ).
Scientific Program
Preliminary Scientific Program:
- Solar Interior and Dynamo
- Quiet-Sun Photosphere - Nonmagnetic and Magnetic Aspects
- Chromosphere and Spicules, Prominences
- Transition Region and Corona
- Sunspots and Active Regions
- Flares and Magnetic Helicity
- 3D Structure of the Outer Atmosphere
- CME Source Regions and Interplanetary CMEs
- Solar Wind and the Interplanetary Space
- Possible Anomaly of the Current Solar Cycle
- Outlook for the Future
Special Session (probably between Sessions 4 and 5):
60 years of Norikura Solar Observatory, NAOJ
Important Dates
- First announcement: 1 Jun, 2009
- Early bird registration deadline: TBA
- Registration deadline: TBA
- Abstract submission deadline: TBA
- Hotel Reservation deadline: TBA
Registration
TBA
Accommodations
TBA