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1)  force-free field
无力场
1.
Using the multistep implicit scheme,a numerical study was made to reveal the influence of linear force-free field to the spontaneous reconnection of current sheets.
采用二维三分量磁流体力学数值模拟方法,研究了线性无力场对电流片的自发重联的影响。
2.
We have introduced in detail main methods of solving solar linear force-free field models,discussed their advantages and disadvantages and understood fully the relations of themethods.
对线性无力场模型的主要求解方法做了详细的介绍,在此基础上分析讨论了各方法的优缺点,并彻底搞清了这些方法之间的内在联系。
2)  Force-free magnetic field
无力磁场
3)  reactive power market
无功电力市场
1.
Reactive Power Ancillary Service and Its Pricing Based on the Model of Optimal Consolidated Compensation Reactive Power Market;
统一优化补偿型无功电力市场下无功功率辅助服务及其定价研究
2.
First, reactive power market and the relevant element are introduced, and then several different frameworks on reactive power market and methods on reactive power pricing are presented and their advantage also defect is summarized.
本文首先对无功电力市场及其相关要素做了介绍。
4)  Solar force-free magnetic field
太阳无力磁场
5)  Force field
力场
1.
Predictions of thermodynamics parameters based on first-principle force field methods;
基于第一原理力场预测热力学参数的探讨
2.
Investigation of H-bonding for the related force fields in materials studio software;
Materials Studio软件涉及力场中氢键的研究
3.
Force Field Method and Thermodynamic Properties Prediction
分子力场方法及热力学性质的预测
6)  field of force
力场
1.
The connotation of Three-yuan field,field of force, electric field and magnetic field is analy-sised respectively and then their different features are pointed out and the study of Three-yuan field via scientific simulation is suggested.
对三元场和力场、电场、磁场等的内涵进行了分析,指出其不同特征,并提出运用现代科学模拟的方法对三元场进行研究。
2.
In order to enhance the research and development of the particle system in teaching and practice of 3ds Max,a method was put forward to use dynamic map and field of force to control the particle emissions and the relation was researched.
为在3ds Max教学与实践中对粒子系统功能的进一步研究与开发,提出了动态贴图和力场控制粒子发射的方法,并对动态贴图、力场、粒子系统三者的关系进行了研究。
补充资料:无力场
      电流方向与磁场平行,因而电磁力为零的磁场,又称无作用力磁场。对携带强磁场的稀薄气体,要维持这种磁场,只有在其气体压力远小于磁压力,而电磁体积力又处处为零的情况下才有可能。磁场为无力场的充分必要条件是墷×B=α(r,t)B,其中B 为磁场强度,α为无力因子,通常是空间位置r和时间t的函数。无力因子α为常数值的磁场是无力场的一种特殊情况,称为稳定无力场。一团受强磁场约束的稀薄导电气体,无论其系统的初始状态如何,只要 α不是常数,这个系统就是不稳定的。但经过演化而趋于稳定时,这时系统的势能,也就是磁能趋于最小状态,即成为稳定无力场。在太阳色球层,由于气体稀薄,气体压力和重力远小于磁压力,色球气体处于稳定状态,其磁场属于无力场。在研究天体磁场时,只要所研究的区域不是处于激烈的活动状态,其瞬时的磁场形态均可以近似地用α 为某一常数值的无力场来表示。
  

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