Changeset 7136
 Timestamp:
 May 30, 2009, 10:30:01 AM (14 years ago)
 Location:
 anuga_core/documentation/user_manual
 Files:

 2 edited
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anuga_core/documentation/user_manual/anuga_user_manual.tex
r7135 r7136 3663 3663 In general, for multiples of the minimal depth $N H_0$ one obtains 3664 3664 \[ 3665 \begin{equation} 3665 3666 \left[ \frac{\mu}{h + h_0/h} \right]_{h = N H_0} = 3666 \frac{\mu}{H_0 (1 + 1/N^2)} 3667 \] 3667 \frac{\mu}{N H_0 + H_0/N} = 3668 \frac{\mu}{h (1 + 1/N^2)} 3669 \label{eq:flux limit multiple} 3670 \end{equation} 3668 3671 which converges quadratically to the true value with the multiple N. 3672 3673 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. 3674 According to Equation \ref{eq:flux limit multiple} this cutoff 3675 affects the calculated velocity by less than 1 \%. 3669 3676 3670 3677 %The developed numerical model has been applied to several test cases 
anuga_core/documentation/user_manual/copyright.tex
r7124 r7136 86 86 \begin{itemize} 87 87 \item John Jakeman, Rudy van Drie, Ted Rigby, Petar Milevski, Joaquim Luis, Nils Goseberg, William Power, 88 Petar Milevski,Trevor Dhu, Linda Stals, Matt Hardy, Jack Kelly and Christopher88 Trevor Dhu, Linda Stals, Matt Hardy, Jack Kelly and Christopher 89 89 Zoppou who contributed to this project at various times. 90 90 \item A stand alone visualiser (anuga\_viewer) based on Openscenegraph was developed by Darran Edmundson.
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