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Some questions about the theory paper of CESE method (doi:10.1006/jcph.1995.1137) #3

@yuhow

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@yuhow

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.

  1. Why does Eq. (2.4) imply Eq. (2.5).?
  2. 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.
  3. (In page 301) What's the finite-difference approximation?
  4. (In page 301) What's the meaning of "the alpha-mu scheme uses a mesh that is staggered in time"?
  5. (In page 301) What's the Lax scheme?
  6. (In page 301) What's the amplification factors? Also what's their meaning/usage in the Leapfrog/DuFort-Frankel scheme?
  7. (In page 301) What's the meaning of "two-level" and "three-level" scheme?
  8. Why does not solutions of Eq. (2.22) dissipate with time? Or why is "no dissipation" equivalent to "neutrally stable"?
  9. Why is the total flux leaving any conservation element zero? This question is relevant to the definition of Eq. (2.28).
  10. Why does the term of second order partial derivative w.r.t. x vanish in Eq. (2.29)?
  11. 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.
  12. (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?
  13. (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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