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2018 ◽  
Vol 142 ◽  
pp. 02008
Author(s):  
Songlin Chen ◽  
Juntao Wang ◽  
Lin Yuan ◽  
Quanyou Li

In order to restrain cement kiln shell’s thermal loss and potential safety hazard, composite design is employed of working layer, thermal-preservation layer and thermal insulation layer. Thermal-preservation layer’s boundary and strain is analyzed and overall thermal conductivity is calculated. The result shows that sinusoidal curve boundary combination between working layer and thermal-preservation layer, slopeshape with angle of 135 degrees between thermal-preservation layer and thermal insulation layer could relieve strain concentration. Composite mullite brick comprehensive thermal conductivity decreases from the working layer 2.74W·m-1·K-1 to 1.50W·m-1·K-1. When applied in cement kiln, temperature of kiln shell is lower 50°C to 70°C than using normal bricks.


2012 ◽  
Vol 542-543 ◽  
pp. 1430-1433
Author(s):  
Wen Liang Xiang ◽  
Xian Guang Luo ◽  
Ye Bin Bi

A visualization algorithm was presented for the optimization of geometrical shape matching in the wheel-rail contact system. The algorithm of the subsection cubic spline interpolation was adopted to fit the wheel-rail profiles curves, and curve boundary was got by the finite difference method; furthermore, the wheel-rail contact positions were figured out by computing the roll angles of wheelset iteratively with the dichotomy. Based on MATLAB and Visual C++, the wheel-rail contact geometrical parameters were calculated and visualized, the simulation results show the algorithm has the strong robustness.


2000 ◽  
Vol 214 (1-2) ◽  
pp. 130-138 ◽  
Author(s):  
G.J. Parker ◽  
C. Cerjan ◽  
D.W. Hewett

1991 ◽  
Vol 148 ◽  
pp. 475-477
Author(s):  
Slobodan Ninkovic ◽  
Miroslav Filipovic

We use a simple, spherically symmetric model for the Galaxy based on the rotation curve for the inner parts. We extrapolate beyond the rotation curve boundary, assuming a dark corona whose total mass is a model parameter. For each mass value assume we calculate the allowed angular-momentum interval for which a cloud is neither tidally disrupted, nor escapes. On the basis of this investigation we reach a conclusion about the expected mass of the Galaxy.


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