In the 2nd Solar-B science meeting science goals, targets of observation,  methods
of observation shall seriously be discussed under the current instrument design. The
new science outputs from Solar-B are central issues of the discussion.  To achieve
the Solar-B science goals,  the software developments for Solar-B operation and
data analysis will also be discussed.
 

Meeting Schedule

The revised schedule is as follows:
 

REQUEST TO SPEAKERS:

LOC requests all speakers to prepare a copy of viewgraphs for proceedings.
Please leave the copy on the reception desk before the end of meeting.

When a speaker prepares PC presentation,

 (1) LOC can get the file from your anonymous ftp site,
     or
 (2) the speaker can send the file to loc@solar.isas.ac.jp as an attachment
      file if the file size is not huge.

 LOC prefers the former to latter.
 

Call for Poster:

LOC prepares A0 size poster boards for participants. Both instrument introduction
and science work are welcome. Please use this opportunity for good discussion.
 
 

	2nd SOLAR-B SCIENCE MEETING    December 4-6, 2000   (Preliminary)
		Name	Affiliation
Dec. 4 (Mon)
09:30-09:40	Welcoming and Introductory Comments	T. Kosugi	ISAS
	<Mission Objectives and Instrument Performance> Chair: T. Watanabe
09:40-10:20	Solar-B Science Objectives  (Overview of the Mission)	K. Shibata	Kyoto Univ.
10:20-10:40	SOT Science Objectives	A. Title	Lockheed
10:40-10:55	Expected Performance of OTA/SOT	Y. Suematsu	NAOJ
10:55-11:15	FPP/SOT Performance and Operations	T. Tarbell	Lockheed
11:15-11:35	XRT Science Objectives	L. Golub	SAO
11:35-11:55	XRT Overview & Operations	E. DeLuca	SAO
11:55-12:15	EIS Science Objectives	L. Culhane	MSSL
12:15-12:35	EIS Performance & Operations	L. Harra	MSSL
12:35-13:40	Lunch
	<High Precision Measurements on Photosphere & Chromosphere> Chair: A. Title
13:40-14:00	Accuracy of the Magnetic Field Measurements and Scientific Targets of SOT	K. Ichimoto	NAOJ
14:00-14:20	Measurements of Small-scale Photospheric Magnetic Fields	T. Berger	Lockheed
14:20-14:50	Magnetic Fields in Active & Quiet Sun	B. Lites	HAO
14:50-15:10	Observations of the Chromosphere with SOT	Y. Hanaoka	NAOJ
15:10-15:30	Wave Propagation through a Magnetized Solar Atmosphere	T. Bogdan	HAO
15:30-15:40	Break
15:40-16:10	Local-Area Helioseismology with SOT	T. Sekii	NAOJ
16:10-16:40	3D MHD Simulation Based on Precision Vector Magnetic                  Field Observations	K. Kusano	Hiroshima U.
Dec 5 (Tue)	<Structure, Dynamics, and Heating of Upper Solar Atmospheres> Chair: L. Golub
09:30-09:50	Observations of Horizontal Magnetic Fields in the Upper Atmosphere with TRACE and Solar-B	A. Title	Lockheed
09:50-10:05	Spicule Observations: What's Needed from Solar-B	A. Sterling	MSFC
10:05-10:25	Quiet Sun Observations with XRT	A. Winebarger	SAO
10:25-10:45	CDS observations of active region loops	E. Landi	NRL
10:45-11:05	Spectral diagnostics and the structure of the outer solar atmosphere	V. Hansteen	Oslo Univ.
11:05-11:25	Coordinated Observations of Magnetic Connections    between Photosphere and Corona by Solar-B    - From La Palma and ASP observations with Yohkoh SXT -	T. Shimizu	NAOJ
11:25-11:45	Observational Constraints for Coronal Heating    - Perspectives from Yohkoh -	S. Nagata	ISAS
11:45-12:05	Observational Constraints for Coronal Heating   - Perspectives from TRACE -	M. Aschwanden	Lockheed
12:05-12:25	Coronal Heating by Small-Scale Energy Release   - Possibility of Nanoflare Heating -	Y. Katsukawa	Univ. Tokyo
12:25-12:40	Coronal Heating from the Magnetic Network	R. Moore	MSFC
12:40-13:40	Lunch
	<Structure, Dynamics, and Heating of Upper Solar Atmospheres; Continued> Chair: G. Doschek
13:40-14:00	Energetics & Velocity Field in the Low Corona	T. Watanabe	NAOJ
14:00-14:20	Origin of Slow Solar Wind	M. Kojima	STE
	<Energetic Events: Flares and CME> Chair: G. Doschek
14:20-14:35	Coronal Velocity Observations around a Flare Loop	K. Ichimoto	NAOJ
14:35-14:55	Dynamics of Solar X-ray Jets	M. Shimojo	NAOJ
14:55-15:25	Recent Progress in Flare/CME Physics	T. Forbes	UNH
15:25-15:35	Break
15:35-15:50	High-Temperature Regions above Solar Flare Loops	S. Akiyama	GU
15:50-16:10	X-Flares Observed with TRACE	K. Reeves	SAO
16:10-16:30	Twisted structures of emerging magnetic ropes to cause solar explosive phenomena	H. Kurokawa et al.	Kyoto Univ.
Dec 6 (Wed)	<Energetic Events: Flares and CME; Continued>  Chair: L. Culhane
09:30-09:50	Evidence for Pre-Flare Activity: Observations From TRACE	H. Warren	SAO
09:50-10:10	Flare Blasts and Dark Filament Rises Leading to the Wave Fronts  in the Low Corona and to Different Types of CME's	Y. Uchida et al.	TSU
10:10-10:30	Non-thermal Velocity Evolution in the Precursor Phase  of a Solar Flare	L. Harra	MSSL
10:30-10:50	Hard X-ray Two Ribbon Flare Observed with Yohkoh/HXT	S. Masuda	STE
10:50-11:10	Studies of Magnetic Reconnection by Solar-B	T. Yokoyama	NAOJ
	<Summary of Science Session>
11:10-11:40	Review of Science with Solar-B	S. Tsuneta	NAOJ
11:40-11:50	Break
	<Operations and Planning of Coordinated Observations> Chair: J. Davis
11:50-12:10	Coordinated Observations among Instruments in a single Satellite         - SOHO Experience -	D. Pike	RAL
12:10-12:30	Target Selection and  Coordinated Observations  with Ground-Based  Observatories  - Trace Experience with Small FOV Instrument -	T. Tarbell	Lockheed
12:30-12:50	Relationship between Solar-B and Ground-Based Observatories	R. Kitai	Kyoto Univ.
12:50-13:50	Lunch
13:50-14:10	Target Selection in Solar-B Operations	T. Sakao	ISAS
14:10-14:30	Create Solar-B Sample Timeline (eg. Synoptic Observations)	H. Hara	NAOJ
14:30-14:50	Sample Plan for Usage of Solar-B Data Recorder	K. Matsuzaki	ISAS
	<Programmatics>
14:50-15:10	Project Status Report (Japan/US/UK)	T. Kosugi L. Hill L. Culhane	ISAS MSFC MSSL
15:10-16:30	Operations and Planning (DISCUSSION)	T. Kosugi	ISAS
	Planning & planning software       Data formats and processing software       Data reduction, analysis and archiving
	Data Policy
	Next Science Meeting

L. Culhane, J. Davis, G. Doschek, L. Golub, T. Kosugi, T. Sakurai, K. Shibata, A. Title

Local Organizing Committee:

K. Daiguji, H. Hara, T. Kosugi, K. Matsuzaki, T. Sakao
 

Date:    Dec 4 - 6, 2000
Place: Film Center, Sagamihara, Tokyo: located just in front of the ISAS gate
            It is 15 min walking distance to get to Film Center from Fuchinobe station.

Equipments for Presentation:

Overhead projector, PC projector, and VHS video projector are available.
 
 

Contact:

If you have some requests and questions, please contact Miss Daiguji or
Hara. Miss Daiguji will help you for the hotel reservation.

H. Hara      : hara@solar.mtk.nao.ac.jp
K. Daiguji    : daiguji@laputa2.solar.isas.ac.jp

TEL: +81-(0)427-59-8175  (Dr. Kosugi's office)
FAX: +81-(0)427-59-8457 (Please add 'To Dr. Kosugi's office'at the top)
 

Hotel Information:

Please Find your hotel !   List of Foreign Participants
 
 

Sagamihara Daiichi Hotel

Phone:            +81-(0)42-751-6551
Fax:                +81-(0)42-751-4643
Room Charge:   JY 6,510/night (single room: including tax)
                      (Breakfast is available but at an additional cost of JY 900.)
Check-in time:  3:00 PM

The hotel is located within a 2-minute walking distance from Fuchinobe
station. You can see the hotel to the right-hand side (north-east direction)
from the station's north exit.

The hotel accepts most of major credit cards such as JCB, VISA, AMEX,
DC, and BANKS. You are requested to pay room charges when checking-in.

We've informed the hotel front expected arrival time of yours for avoiding
any problems. The hotel front is open 24 hours. However, please be advized
to call the hotel in case when your scheduled arrival time delays by more
than a few hours.
 

Central Hotel Machida

Phone: +81-(0)427-20-3011
FAX:    +81-(0)427-20-3022

Check-in time: 3:00 PM

The hotel is located within a 2-minute walking distance from Machida
station.

Hotel Mets Musashisakai

Phone: +81-(0)422-32-5111
FAX:    +81-(0)422-32-5100

Check-in time: 3:00 PM
 

Route map:
 
 

From Narita Airport to Fuchuinobe Station: