期刊文献+
共找到3篇文章
< 1 >
每页显示 20 50 100
Auxiliary error and probability density function based neuro-fuzzy model and its application in batch processes
1
作者 贾立 袁凯 《Chinese Journal of Chemical Engineering》 SCIE EI CAS CSCD 2015年第12期2013-2019,共7页
This paper focuses on resolving the identification problem of a neuro-fuzzy model(NFM) applied in batch processes. A hybrid learning algorithm is introduced to identify the proposed NFM with the idea of auxiliary erro... This paper focuses on resolving the identification problem of a neuro-fuzzy model(NFM) applied in batch processes. A hybrid learning algorithm is introduced to identify the proposed NFM with the idea of auxiliary error model and the identification principle based on the probability density function(PDF). The main contribution is that the NFM parameter updating approach is transformed into the shape control for the PDF of modeling error. More specifically, a virtual adaptive control system is constructed with the aid of the auxiliary error model and then the PDF shape control idea is used to tune NFM parameters so that the PDF of modeling error is controlled to follow a targeted PDF, which is in Gaussian or uniform distribution. Examples are used to validate the applicability of the proposed method and comparisons are made with the minimum mean square error based approaches. 展开更多
关键词 Batch process Auxiliary error model Probability density function Neuro-fuzzy model
下载PDF
1998年物探年度综述
2
作者 崔林沛 《国土资源科技进展》 2000年第1期46-47,共2页
地面物探通常用来寻找和圈定矿体.而物探作为获得基础地质信息的经济合算的手段,其作用往往被低估。Lowe等人在加拿大温哥华岛北部所做的地质调查清楚地证明了这一点,他们采用了重力、磁测、电磁和地震折射法。两个不同地点的结果给... 地面物探通常用来寻找和圈定矿体.而物探作为获得基础地质信息的经济合算的手段,其作用往往被低估。Lowe等人在加拿大温哥华岛北部所做的地质调查清楚地证明了这一点,他们采用了重力、磁测、电磁和地震折射法。两个不同地点的结果给出了地下的详细图象,而成本只有钻探成本的零头。在Rupert湾以东的一个地点,他们的模型表明,容矿的Bonanza群的分布不像原来想的那么广。 展开更多
关键词 地面物探 地震折射法 重力数据 密度差模型 矿产勘查
全文增补中
Constraining a New Type of Dark Energy Model from Present Observations
3
作者 谢磊 陈晶晶 +3 位作者 郑蔚玮 夏骏 柳高平 苏奇平 《Communications in Theoretical Physics》 SCIE CAS CSCD 2013年第2期249-252,共4页
We propose a new type of dark energy (DE) model, in which the equation of state of DE wae is a simple function of the fractional energy density Ωde instead of the redshift z. We assume three DE models of this type,... We propose a new type of dark energy (DE) model, in which the equation of state of DE wae is a simple function of the fractional energy density Ωde instead of the redshift z. We assume three DE models of this type, and fit them with present observations to get constraints of DE, which are also compared with the CPL model. It is shown that a suitable wda,(Ωde) model can give smaller X2 or smaller errors of wde than that of the CPL model. This new type of DE model can help to study the essential properties and nature of DE. 展开更多
关键词 dark energy PARAMETRIZATION cosmological model
原文传递
上一页 1 下一页 到第
使用帮助 返回顶部