核聚變溫度 的英文怎麼說
中文拼音 [héjùbiànwēndù]
核聚變溫度
英文
fusion point-
In this paper, the course of isothermal crystallization kinetics of polymer in limited volume unit is simulated by use of the method of monte carlo. four factors influenting on the course of polymer in the limited volume unite isothermal crystallization are analyzed under the given conditions. the four factors are sample volume shrinkage, the change of the linear growth rate of entities g, the change of sample thickness and the change of the number of nuclei
本文採用montecarlo方法研究了高聚物在有限體積元中的等溫結晶動力學過程，分析了在一定條件下，樣品體積收縮、晶體線生長速率變化、樣品厚度變化和晶核數目變化這四種因素對高聚物在有限體積元中的等溫結晶過程的影響。H. moreover, high density is required to increase the chance of collision. hence, the reactions can only take place in the core of the sun, with temperature over ten million degrees 10
首先核聚變需要極高的溫度，讓氫原子核能有足夠的能量克服原子核之間的電排斥力，此外亦需要極高的密度去增加粒子碰撞的機會，所以核聚變只能在溫度高達10If the mass of the star is less than about 1. 1 solar masses, the temperature of the core will be less than 15 million k, the main fusion reaction is the
若星體質量小於太陽質量的1 . 1倍，星體中心的溫度將會少於一千五百萬絕對溫度，核聚變主要以Main content in simulation is the spatio - temporal evolution of the set of descriptive variables characterizing tectonic mineralization state under coupling of various processes as following : ( 1 ) variables related to forming and property of ore - forming fluid, such as dissolution rate of minerals ( include metal minerals ) in rock, concentration and saturation of aqueous species in fluid, temperature, pressure, and ionic strength etc. ; ( 2 ) variables related to structural deformation and fluid flow, such as stress, deformation rate, fracture network, porosity, fracture permeability ; ( 3 ) variables related to precipitation and mineralization, such as nucleation rate of gangue and metal minerals, accumulation precipitation of various minerals, etc. ; ( 4 ) spatio - temporal coupling relation of various variables above, such as the coupling relationship between spatio - temporal evolution of fracture permeability and flow and focus of fluid and ore - forming
模擬的主要內容是在各種過程耦合作用下，以下描述構造成礦體系的主要變量的時空演化：與成礦流體的形成和性質有關的變量，如地層中礦物（包括成礦物質）的溶解速率、流體中各組分的濃度與飽和度、流體溫度、壓力、離子強度等；與構造變形和流體運移有關的各變量，如應力與變形速率、巖石孔隙度、構造（斷裂）滲透率等；與沉澱成礦有關的變量，如礦物（金屬礦物和脈石礦物）的成核速率、各礦物的沉澱量等；上述各有關變量間的時空耦合關系，如斷裂滲透率時空演化與流體流動、匯聚和成礦的耦合關系等。The core meanwhile will reach a temperature of 100 million degrees kelvin, and the helium nuclei will begin fusing into carbon nuclei
在此期間核心溫度會達到1億k ，氦原子核將開始聚變成碳原子核。In earlier times, jupiter may have been hot enough to have been glowing as an infrared heat source, that affected the evolution of the moons of jupiter
對于木星這樣低的核心溫度，其內部的核聚變概率小到根本不可能產生任何可測量的變化！分享友人