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Some questions about the theory paper of CESE method (doi:10.1006/jcph.1995.1137) #3
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When referring to a term in a page, please also indicate which line and paragraph it is. Or, quote the context in the question. It will save reviewers' time.
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Thanks for your reply! Why can "Eq. (2.19)" be proved using the fact that the total flux of h* leaving the boundary of any space-time region that is the union of any combination of CEs vanishes? Can't figure it out. It should be Eq. (2.19). Sorry for misleading you. And sorry for the lack of information in Q12: (In page 304) Why is the local convective motion of physical variables relative to the moving mesh kept to a minimum if the space-time mesh is allowed to evolve with the physical variables? The relevant description is in the end of bullet (a) at the second-last paragraph of the left column in page 304. |
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Few more questions from Section 5 (The Euler Solver):
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The parts you read is about designing weighting functions for treating discontinuities. It's complex. Many of the techniques are developed with experiences and can be ad hoc. They are necessary for treating strong non-linear equations like the Euler equations, in which shocks exist.
To more understand the discontinuity treatments, you need to experiment with various settings in a code. It becomes simple how You can read the whole theory in Courant76 and Lax73. But I suggest you to finish all the coding before reading it. The theory of conservation laws takes more time to digest than the CESE method itself. |
Dear all,
The following message is some of my questions about the alpha-mu scheme in the theory paper of CESE method (doi:10.1006/jcph.1995.1137)
Basically, all the following questions are based on the Section 2 (alpha-mu scheme) of the paper.
Please help me. So many thanks in advance.
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