实现受控热核聚变反应的两个最基本问题就是-计算机应用研究室

1、J Jacquinot, Geneva FEC 2008,1,JJ OCS Cannes 17 March 08,1,50 years in Fusionandthe Way Forward,1026 watts, 0.01 W/m3,5.108 watts, 5 105 W/m3,J Jacquinot, FEC 2008,J Jacquinot, Geneva FEC 2008,2,Credits,Discussions with many colleagues and direct input from: R. Arnoux, H. Azechi, B. Bigot; D. Besnar

2、d, S. Bourmaud, J. Ebrardt, Ph. Ghendrih, M. Kikuchi, R. Stambaugh, G. Mank, A. Malaquias, D. Meade, E. Oktay, M. Skoric, Q. Tran, H. Yamada,Case for fusion Key milestones Lessons from the past The way forward,J Jacquinot, Geneva FEC 2008,3,JJ OCS Cannes 17 March 08,3,Today: 80 % of primary energy c

3、omes from fossil resources Gas global stability 1990 2000+ Scaling laws Fusion for real Tok: Pfus 10MW; 51018 neutrons Tok + Stel: Duration minutes IF: 600 times liquid, 10keV, 2x1013 neutrons 2000 to present Start of a new era ITER + BA; NIF global stability 1990 2000+ Scaling laws Fusion for real

4、Tok: Pfus 10MW; 51018 neutrons Tok + Stel: Duration minutes IF: 600 times liquid, 10keV, 2x1013 neutrons 2000 to present Start of a new era ITER + BA; NIF e. g. disruption forces Becoming predominant: Supra conductors Materials Heat transfer Safety Operation in CW or high duty cycle The obvious next

5、 challenge for both MF and IF a new era for engineering!,J Jacquinot, Geneva FEC 2008,59,Lessons from the past : organisation,JET: H. O. Wster to US Congress (1986): “JET could succeed because it was given the power to manage” Organisation: Council sets “What” (objectives present effort enough?,Summary