fusion reactions信息详情
[核]聚变反应;熔合反应
fusion───n.融合;熔化;熔接;融合物;[物]核聚变
reactions───n.[生理][化学][医]反应(reaction的复数)
inertial fusion───惯性聚变
tribal fusion───部落融合
mixed reactions───各种不同反应
fusion food───融合菜;无国界料理
chain reactions───连锁反应;[物化]链式反应;n.连锁反应( chain reaction的名词复数 )
allergic reactions───过敏反应;[免疫]变态反应
emotional reactions───情绪反应(emotionalreaction的复数)
Other fusion reactions do occur quickly enough.───其他的一些核聚变反应却是很快的。
are formed when the nuclear fusion reactions at the centre of a star can no longer support its structure.───是当一个恒星的中心核聚变反应不再能支持其结构时而形成的。
Such fusion reactions will give rise to a great deal of energy to enable the sun to continuously emit light and heat.───和高温作用下,太阳从内至外不断地产生着聚变反应,这种聚变提供了大量的能量使太阳能不断地释放出光和热。
Systems of this sort are being used in an effort to produce controlled thermonuclear fusion reactions.───这类系统正用于产生受控热核聚变反应的探索。
Requiring temperatures of more than 100 million degrees Celsius, the fusion reactions have to be contained in magnetic fields.───聚变反应必须控制在磁场内,需要一亿摄氏度的温度。
So when physicists tell us that stars generate light and heat from nuclear fusion reactions inside the stars, what evidences do they have?───那么,当物理学家告诉我们,恒星藉著内部的核融合反应发光发热,究竟有甚么凭据?
These are formed when the nuclear fusion reactions at the centre of a star can no longer support its structure.───行星状星云是当一个恒星的中心核聚变反应不再能支持其结构时而形成的。
This should, in turn, cause more fusion reactions until the fuel runs out.───这应当依次导致更多的聚变反应,直到燃料耗尽。
Systems of this sort are being used in an effort to produce controlled thermonuclear fusion reactions.
However, fusion reactions on the sun are uncontrollable, just like H-bomb explosion seen on the earth. Huge amount of energy will be produced in a minute, which may be destructive.
The fusion reactions that power the sun must produce vast numbers of neutrinos.
In fusion reactions, light atoms are brought together sufficiently energetically to overcome their natural repulsion.
Nuclear fusion reactions between deuterium ions produced between 10 5 and 10 6 neutrons per pulse.
The cross sections for these fusion reactions are appreciable only for incident energies above 10 KeV.
The first controlled fusion reactions had been seen and their nature was now being clarified.
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