1) entropic variation minimization
熵变分量小化
2) entropy variable
熵变量
1.
The Euler equations of quasi-linear form in conservation variables can be transformed into the Euler equations of symmetric form in entropy variables by introducing the change of variables.
通过变量代换将拟线性守恒变最欧拉方程组转换为具有对称性的熵变量欧拉方程组，对该方程组构造ＳＵＰＧ的弱解式，其中权函数摄动项中包含流向算子和间断捕获算子。
3) entropy minimization
熵最小化
4) entropy variation
熵变分
1.
An image denoising model based on entropy variation is proposed from the viewpoint of maximum a posteriori probabilities(MAP) and maximum entropy theory.
针对传统Tikhonov正则化模型存在的不足,根据最大后验概率(MAP)和最大熵的理论,提出了一种基于熵变分的图像去噪模型。
5) magnetic entropy change
磁熵变化
1.
From the measurement and calculation of magnetization under various temperatures, we have discovered large magnetocaloric effect with the ferromagnetic-paramagnetic transition, additional magnetism exchange action introduces additional magnetic entropy change.
通过不同温度下的等温磁化(M-H)曲线的测量和计算,发现伴随铁磁-顺磁(PM-FM)相变出现大的磁热效应,额外的磁性交换作用将导致额外的磁熵变化。
2.
From the measurement and calculation of magnetization under various temperatures, we have discovered large magnetocaloric effect with the ferromagnetic paramagnetic transition, additional magnetism exchange action introduces additional magnetic entropy change.
3MnO3的磁热效应进行了研究 ,通过不同温度下的等温磁化 (M H)曲线的测量和计算 ,发现伴随铁磁 顺磁相变出现大的磁热效应 ,额外的磁性交换作用将导致额外的磁熵变化 。
6) change rate of entropy
熵变化率
1.
As an example of non-stationary black holes,the relationship between the compression factor of time scale near the event horizon and the temperature as well as the change rate of entropy of the Vaidya black hole is researched.
研究了动态黑洞的温度、熵变化率与事件视界附近“时间尺度压缩因子”之间的关系。
补充资料：公理化方法(见公理化和形式化)
公理化方法(见公理化和形式化)
axiomatical method
gongllbuafangfa公理化方法化和形式化。(axiomatieal method)见公理
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条