T. Sato – författare

20 years after the collapse of communism in Central Eastern European countries and 30 years after the start of market-oriented reforms in China, this book provides a framework for understanding the differing emphasis and sequencing of two reforms and explores in-depth these issues in the demise of communism and the triumph of the market economy.

20 years after the collapse of communism in Central Eastern European countries and 30 years after the start of market-oriented reforms in China, this book provides a framework for understanding the differing emphasis and sequencing of two reforms and explores in-depth these issues in the demise of communism and the triumph of the market economy.

20 years after the collapse of communism in Central Eastern European countries and 30 years after the start of market-oriented reforms in China, this book provides a framework for understanding the differing emphasis and sequencing of two reforms and explores in-depth these issues in the demise of communism and the triumph of the market economy.

Computer simulation is now widely recognized as a powerful tool and useful method at the current stage of research in space plasma physics. The expected role of computer simulation is to bridge the existing gap between theories and experiments/observations and to give a profound physical insight into highly tangled and nonlinearly coupled space plasma phenomena. One of the goals of space plasma physics in 1980's and 1990's is to elucidate the quantitative causal relationships of global and local energy flows in space plasma environment and establish the space plasma physics via cooperative studies among three important elements of observations, theories and computer simulations. Based on such recognition, Dr. M. Ashour-Abdalla (UCLA/USA), Dr. R. Gendrin (CNET/FRANCE) and both of us met together at the 20th General Assembly of URSI at Washington D. C. in 1981 to discuss what we should do and what we could do, reaching a conclusion that it is time to establish an International School of Space Simulations (ISSS). The objectives of the ISSS thus organized are firstly to educate and stimulate graduate students and young sCientists, secondly to exchange information on updated simulation techniques and thirdly to have mutual discussions among observational, theoretical and simulational scientists in the field of space physics. The first ISSS were organized by Prof. P. Coleman, Prof. T. Obayashi, Dr. H. Okuda in addition to the above four members. The first ISSS was held at Kansai Seminar House in Kyoto from Nov. I to Nov. 12, 1982.

The purpose of the symposium is to discuss current experimental and theoretical studies of weak and electromagnetic interactions in nuclei, emphasizing fundamental problems of particle, nuclear and astrophysics. Subjects discussed included symmetries and conservation laws, neutrino physics, nuclear weak process and weak form factors, electromagnetic probes for hadrons and nuclear structures, symmetries and flavornuclei, new facilities, and others.