Changeset 7124
 Timestamp:
 May 28, 2009, 11:03:22 AM (11 years ago)
 Location:
 anuga_core/documentation/user_manual
 Files:

 2 edited
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anuga_core/documentation/user_manual/anuga_user_manual.tex
r7105 r7124 3352 3352 \] 3353 3353 In general, for multiples of the minimal depth $N H_0$ one obtains 3354 \ [3354 \begin{equation} 3355 3355 \left[ \frac{\mu}{h + h_0/h} \right]_{h = N H_0} = 3356 \frac{\mu}{H_0 (1 + 1/N^2)} 3357 \] 3356 \frac{\mu}{N H_0 + H_0/N} = 3357 \frac{\mu}{h (1 + 1/N^2)} 3358 \label{eq:flux limit multiple} 3359 \end{equation} 3358 3360 which converges quadratically to the true value with the multiple N. 3361 3362 Although this equation can be used for any depth, we have restricted its use to depths less than $10 * H_0$ (or 1 cm) to computational resources. 3363 According to Equation \ref{eq:flux limit multiple} this cutoff 3364 affects the calculated velocity by less than 1 \%. 3359 3365 3360 3366 %The developed numerical model has been applied to several test cases 
anuga_core/documentation/user_manual/copyright.tex
r7064 r7124 85 85 \textbf{Acknowledgments}: 86 86 \begin{itemize} 87 \item John Jakeman, Rudy van Drie, Ted Rigby, Joaquim Luis, Nils Goseberg, William Power,87 \item John Jakeman, Rudy van Drie, Ted Rigby, Petar Milevski, Joaquim Luis, Nils Goseberg, William Power, 88 88 Petar Milevski, Trevor Dhu, Linda Stals, Matt Hardy, Jack Kelly and Christopher 89 89 Zoppou who contributed to this project at various times.
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