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Some questions about the theory paper of CESE method (doi:10.1006/jcph.1995.1137) #3
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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.
- Why does Eq. (2.4) imply Eq. (2.5).?
- Why can Eq. (2.9) 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.
- (In page 301) What's the finite-difference approximation?
- (In page 301) What's the meaning of "the alpha-mu scheme uses a mesh that is staggered in time"?
- (In page 301) What's the Lax scheme?
- (In page 301) What's the amplification factors? Also what's their meaning/usage in the Leapfrog/DuFort-Frankel scheme?
- (In page 301) What's the meaning of "two-level" and "three-level" scheme?
- Why does not solutions of Eq. (2.22) dissipate with time? Or why is "no dissipation" equivalent to "neutrally stable"?
- Why is the total flux leaving any conservation element zero? This question is relevant to the definition of Eq. (2.28).
- Why does the term of second order partial derivative w.r.t. x vanish in Eq. (2.29)?
- Eq. (2.33) maybe is wrong. The partial derivative in the left-hand side of Eq. (2.33) should be with respect to x instead of t.
- (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?
- (In page 304) What's the meaning of "principal" and "spurious" amplification factors?
Please help me. So many thanks in advance.
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