Dear Participants of the Nobeyama symposium 2004,

Attached below, please find the second circular of the symposium.  For
further communication, please send your message NOT to shibasaki@NRO
but to nbym04@NRO.  Shibasaki will be absent for a couple of days next
week.

*To those who have not yet submitted abstracts, please send them to
nbym04@NRO.
*To those who have not yet informed us detailed flight schedule, and/or
not yet sent us copies of air ticket, please inform us and send them
to us by e-mail or by FAX (+81-267-98-2506).

Please visit agian the meeting web page
(http://solar.nro.nao.ac.jp/meeting/nbym04/) and read carefully the
Papaerlist, which is the list of published papers which include
Nobeyama Radioheliograph data or results.  If you noticed missing
papers, please inform us (nbym04@NRO).  Also please bring two copies
of your proceedings papers for our archives.

Looking forward to meeting you soon at Kiyosato.

Kiyoto
(NRO: nro.nao.ac.jp)
***************************** Second circular ***************************** 

"Solar Physics with the Nobeyama Radioheliograph"
            (Nobeyama Symposium 2004) 
    http://solar.nro.nao.ac.jp/meeting/nbym04/

Date : 2004 October 26 (Tue.) - 29 (Fri.)
Venue: Seisenryo at Kiyosato 
SOC  : T. Bastian, N. Gopalswamy, T. Kosugi, K. Shibasaki(chair), T. Yokoyama
LOC  : A. Asai, H. Kodama, K.Shibasaki(chair), M. Shimojo  
       nbym04@NRO (NRO:nro.nao.ac.jp)

Objective of the meeting:
 Nobeyama Radioheliograph (NoRH) has been observing the Sun for more
than 12 years.  We completed one solar cycle of observations.  To mark
this occasion, we want to summarize what has been done with the
heliograph and to discuss what we should do in the future.  Papers to
be presentied in the meeting will be mainly concerned with the results
from the NoRH, closely related field and future plans.

Meeting Venue:
 The Nobeyama Symposium 2004 will be held at SEISEN-RYO at Kiyosato,
which is located near Nobeyama Solar Radio Observatory.  All
participants are expected to stay at
Seisen-Ryo. http://www.keep.or.jp/indexe.html

Access:
 Access to NRO and Map 
   http://www.nro.nao.ac.jp/Info/gettoNRO-e.html
 Access to NAOJ(Mitaka) and Map (Access to Cosmos-Kaikan) 
   http://www.nao.ac.jp/Map/index.html

Time Tables:
 from Narita to Kiyosato 
   http://solar.nro.nao.ac.jp/meeting/nbym04/nari-kiyo.htm
 from Kiyosato to Narita 
   http://solar.nro.nao.ac.jp/meeting/nbym04/kiyo-nari.htm
 from Niigata to Nobeyama / from Nobeyama to Niigata 
   http://solar.nro.nao.ac.jp/meeting/nbym04/nii-nobe.htm
 from Narita to Shinjuku
   http://www.jreast.co.jp/nex/e_TimeTable/e_sobu_narita_u/e_sobu_narita2_u/index.html
 from Shinjuku to Narita 
   http://www.jreast.co.jp/nex/e_TimeTable/e_sobu_narita_d/e_sobu_narita2_d/index.html

Internet Service:
Internet connection (with DHCP) is available in Seisen-Ryo. We will
provide ethernet cables (RJ45), HUBs, but no Wireless LAN.

Other Informations and Links:
Seisen-Ryo 
  http://www.keep.or.jp/indexe.html
Weather Information about Kiyosato
  http://www.snowjapan.com/e/resorts/resortdetail.php?resid=200
Takane Town Office (Information about Kiyosato Highland) 
  http://tkn.yatsu.gr.jp/kiyosato/english/index.html
Nobeyama Solar Radio Observatory 
  http://solar.nro.nao.ac.jp/
NAOJ (Mitaka) 
  http://www.nao.ac.jp/E/index.html
Tokyo Narita Airport 
  http://www.narita-airport.or.jp/airport_e/index.html
Niigata Airport 
 http://www.pref.niigata.jp/gateway/english/niigataairport/airportnetwork.htm

Travel support:
 To refund your travel cost during your stay in Kiyosato, we need to
know the actual cost of your air ticket beforehand.  Please send to
LOC (nbym04@NRO) the copy of your ticket (or e-ticket confirmation)
and/or receipt of the payment for the ticket as soon as possible.
Also we will ask you to copy of your ticket and passport at the LOC
office during the meeting.  Room charge and cost of meals will be paid
directly to the hotel.  Extra cost (such as telephone, drinks, etc.)
should be paid by yourself when you checkout.  LOC office will be
located on the 1st floor of the poster session room.

************** Social Program ************** 
Welcome Reception October 25 (Monday) 17:30- at Seisen-Ryo  
Excursion October 28 (Thursday) 14:00- to Nobeyama Radio Observatory  
Banquet October 28 (Thursday) 18:00- Sushi Party at NSRO  

************** Science Program ************** 
October 25 (Monday) 17:30- Welcome Reception at Seisen-Ryo
October 26 (Tuesday)  
09:00 - 9:30  Welcome Address / Introduction (K. Shibasaki)  

09:30 - 12:15  Session I : Flares & Particle Acceleration 1 
                           (Chair : T. Kosugi)  
09:30 - 10:15  Flares and Particle Acceleration 1. (T. Bastian)  
 Coffee Break  
10:45 - 11:15  Flares and Particle Acceleration 2. (V. Melnikov)  
11:15 - 11:45  Flare Associated Oscillations Observed with NoRH (A. Asai)  
11:45 - 12:15  Fine temporal and spatial structure of the microwave emission 
               sources from the SSRT and NoRH observations (A. Altyntsev)  
 Lunch  
14:00 - 17:20  Session II : Flares & Particle Acceleration 2 
                            (Chair : A. Stepanov)  
14:00 - 14:30  Nonthermal Electrons in an Ejecta Associated with a Solar 
               Flare (S. Masuda)  
14:30 - 15:00  Periodic Acceleration of Electrons in Solar Flares (S. Kamio)  
15:00 - 15:30  Moving Magnetic Features, Loop-Loop Interactions and Repeated 
               Flaring (S. Pohjolainen)  
 Coffee Break  
16:00 - 17:20  Poster Presentations (10min * 8)  

October 27 (Wednesday)  
09:00 - 12:15  Session III : Flares & Particle Acceleration 3 
                             (Chair : T. Yokoyama)  
09:00 - 09:30  Energetic Electrons in a Flaring Loop (H. Nakajima)  
09:30 - 10:00  The Spatially Resolved Spectrum Analysis of Gradual Hardening 
               Flare (H. Takasaki)  
10:00 - 10:30  Diagnostics of Flare Plasma Using Pulsations in Microwave and 
               X-ray Emission (A. Stepanov)  
 Coffee Break  
11:00 - 11:45  Overview of RHESSI Results (H. Hudson)  
11:45 - 12:15  NoRH Flare Studies with RHESSI and TRACE (S. White)  
 Lunch  
14:00 - 17:30  Session IV : Flares & Particle Acceleration 4 
                            (Chair : T. Bastian)  
14:00 - 14:30  NoRH Observations of RHESSI Microflares (M. Kundu)  
14:30 - 15:00  RHESSI and NoRH Observations of the 3 July 2002 Flare 
               (K. Hori)  
15:00 - 15:30  Two Years of NoRH and RHESSI Observations: What Have we 
               Learned? (A. Nindos)  
 Coffee Break  
16:00 - 16:30  Gyrosynchrotron Emission from Anisotropic Electron 
               Distributions (G. Fleishman)  
16:30 - 17:00  Radio Signature of Coronal Magnetic Fields and 
               Reconnections (G. Huang)  
17:00 - 17:30  Internal Shocks in the Reconnection Jet in Solar Flares 
               (S. Tanuma)  
October 28 (Thursday)  
09:00 - 11:45  Session V : Eruptive Phenomena & CMEs 
                           (Chair : D. Gary)  
09:00 - 09:45  Radio Observations of Solar Eruptions (N. Gopalswamy)  
09:45 - 10:15  NoRH Observations of Prominence Eruptions (M. Shimojo)  
 Coffee Break  
10:45 - 11:15  Observations of Eruptive Events with Two Radioheliographs, 
               SSRT and NoRH (V. Grechnev)  
11:15 - 11:45  Radio Observations of EIT Waves and Coronal Dimmings 
               (S. White)  
 Lunch  
14:00 -  Excursion to NSRO & Banquet (Sushi Party at NSRO)

October 29 (Friday)  
09:00 - 12:15  Session VI : Quiet Sun & Active Regions 
                            (Chair : S. White) 
09:00 - 09:20  Global Development of the Solar Cycle as Found from the 
               Nobeyama Radio Observations (G. Gelfreikh)  
09:20 - 09:45  Quasi-Periodic Oscillations of the Radio Emission of the 
               Solar Plasma Structures and their Nature (G. Gelfreikh)  
09:45 - 10:15  Quiet Sun and Active Region Studies by Nobeyama 
               Radioheliograph (K. Shibasaki)  
 Coffee Break  
10:45 - 11:15  Observations of Quiet Solar Features with the SSRT and 
               NoRH (V. Grechnev)  
11:15 - 11:45  Coronal Magnetograms of Solar Active Regions Derived 
               from Polarization Inversion in Microwaves (B. Ryabov)  
11:45 - 12:15  Summary (K. Shibasaki)  
 Lunch  
14:00 - 17:30  Session VII : New Projects 
                             (Chair : N. Gopalswamy) 
14:00 - 14:45  FASR Flare Science: Lessons from the Nobeyama 
               Radioheliograph (D. Gary)  
14:45 - 15:30  Solar-B (T. Kosugi)  
 Coffee Break  
16:00 - 17:30  International Heliophysical Year (N. Gopalswamy)  

Poster  (Poster board, H:90 cm, V:180 cm, Please prepare 10 min. presentation)

P1. Observations of a posteruptive arcade on October 22, 2001 with 
    the CORONAS-F/SPIRIT, other spaceborne telescopes, and in 
    microwave (V. Grechnev et al.) 
P2. Some observational conclusions on accelerated electrons in solar 
    flares from Nobeyama, Yohkoh, and other observations (V. Grechnev et al.) 
P3. A method to analyze imaging radio data on solar flares (V. Grechnev) 
P4. On the relation of brightness temperatures in a coronal hole at the 
    wavelengths 5.2 and 1.76 cm (V. Maksimov et al.) 
P5. Mutual Dependence of Physical Variables in Hard X-ray Flares Observed 
    with Yohkoh (T. Minoshima) 
P6. A method to identify the type of a microwave source located anywhere 
    on the solar disk (A. Uralov and G. Rudenko) 
P7. Comparison between Microwave and Hard X-ray Spectral Indices of 
    Temporally and Spatially Resolved Non-Thermal Sources 
    (J. Kiyohara et al.) 
P8. Greenbank Radio Spectrometer (S. White et al.) 
 
List of Participants  

A. Altyntsev (Inst. of Solar-Terrestrial Physics, RUSSIA) 
A. Asai (Nobeyma Solar Radio Observatory, NAOJ, JAPAN) 
T. Bastian (NRAO, USA) 
S. Enome (NAOJ, JAPAN) 
G.D. Fleishman (Ioffe Institute, RUSSIA / NRAO, USA) 
R. Fujii(STEL/Nagoya Univ., JAPAN)
D. Gary (NJIT, USA) 
G.B. Gelfreikh (Pulkovo Astronomical Observatory, RUSSIA) 
N. Gopalswamy (NASA/GSFC, USA) 
V.V. Grechnev (Inst. of Solar-Terrestrial Physics, RUSSIA) 
K. Hori (NiCT, JAPAN) 
G. Huang (Purple Mt. Observatory, CHINA) 
S. Kamio (Kyoto Univ., JAPAN) 
T. Kosugi (ISAS/JAXA, JAPAN) 
H.S. Hudson (SSL/UC Berkeley, USA) 
M.R. Kundu (Univ. of Maryland, USA) 
S. Masuda (STEL/Nagoya Univ., JAPAN) 
V. Melnikov (Radiophysical Research Inst., RUSSIA) 
T. Minoshima (Univ. of Tokyo, JAPAN) 
H. Nakajima (Nobeyama Solar Radio Observatory, NAOJ, JAPAN) 
Y. Namiki (Nobeyama Solar Radio Observatory, NAOJ, JAPAN) 
A. Nindos (Univ. of Ioannina, GREECE) 
M. Nishio (Kagoshima Univ., JAPAN) 
S. Pohjolainen (Univ. of Turku, Finland) 
B.I. Ryabov (Latvian Univ., Latvia) 
T. Sakurai (NAOJ, JAPAN) 
K. Shibasaki (Nobeyama Solar Radio Observatory, NAOJ, JAPAN) 
M. Shimojo (Nobeyama Solar Radio Observatory, NAOJ, JAPAN) 
A.V. Stepanov (Pulkovo Observatory, RUSSIA) 
H. Takasaki (Kyoto Univ., JAPAN) 
S. Tanuma (Kyoto Univ., JAPAN) 
T. Watanabe (NAOJ, JAPAN) 
S.M. White (Univ. of Maryland, USA) 
T. Yokoyama (Univ. of Tokyo, JAPAN) 


Proceedings:
 All the presented electronic material will be published on CD-ROM.
We propose to publish a special issue of PASJ (Publication of
Astronomical Society of Japan) consisting of papers selected by the
SOC at the end of the meeting.  As PASJ accept only original papers,
it is necessary to ask authors to write original papers based on the
material presented at the meeting.  A spacial issue of PASJ requires
more than 10 papers.  Normal refereeing process is required.  Review
papers and the complete list of publications concerned with the
results from the NoRH will be published as a Proceedings book.  We
will ask PASJ editorial board to invite one review paper for the
special issue.

 Please use PASJ templates for preparing original papers and also
review papers (for the proceedings book) and follow the instruction.
Please limit the number of color pages for printing material.  We
suggest page limit of 10 for 30 min. review and 15 for 45 min. review.

 http://www.asj.or.jp/pasj/en/index-E.html
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