--- manual/s_overview/text/manual.tex	2004/10/17 04:15:13	1.22
+++ manual/s_overview/text/manual.tex	2006/04/05 02:27:32	1.24
@@ -1,4 +1,4 @@
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.22 2004/10/17 04:15:13 jmc Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.24 2006/04/05 02:27:32 edhill Exp $
 % $Name:  $
 
 %tci%\documentclass[12pt]{book}
@@ -34,7 +34,7 @@
 
 % Section: Overview
 
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.22 2004/10/17 04:15:13 jmc Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.24 2006/04/05 02:27:32 edhill Exp $
 % $Name:  $
 
 This document provides the reader with the information necessary to
@@ -88,7 +88,7 @@
 \end{itemize}
 
 Key publications reporting on and charting the development of the model are
-\cite{hill:95,marshall:97a,marshall:97b,adcroft:97,marshall:98,adcroft:99,hill:99,maro-eta:99}:
+\cite{hill:95,marshall:97a,marshall:97b,adcroft:97,marshall:98,adcroft:99,hill:99,maro-eta:99,adcroft:04a,adcroft:04b,marshall:04}:
 
 \begin{verbatim}
 Hill, C. and J. Marshall, (1995)
@@ -137,12 +137,12 @@
 We begin by briefly showing some of the results of the model in action to
 give a feel for the wide range of problems that can be addressed using it.
 
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.22 2004/10/17 04:15:13 jmc Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.24 2006/04/05 02:27:32 edhill Exp $
 % $Name:  $
 
 \section{Illustrations of the model in action}
 
-The MITgcm has been designed and used to model a wide range of phenomena,
+MITgcm has been designed and used to model a wide range of phenomena,
 from convection on the scale of meters in the ocean to the global pattern of
 atmospheric winds - see figure \ref{fig:all-scales}. To give a flavor of the
 kinds of problems the model has been used to study, we briefly describe some
@@ -372,7 +372,7 @@
 \input{part1/lab_figure}
 %%CNHend
 
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.22 2004/10/17 04:15:13 jmc Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.24 2006/04/05 02:27:32 edhill Exp $
 % $Name:  $
 
 \section{Continuous equations in `r' coordinates}
@@ -770,15 +770,16 @@
 
 \subsubsection{Shallow atmosphere approximation}
 
-Most models are based on the `hydrostatic primitive equations' (HPE's) in
-which the vertical momentum equation is reduced to a statement of
-hydrostatic balance and the `traditional approximation' is made in which the
-Coriolis force is treated approximately and the shallow atmosphere
-approximation is made.\ The MITgcm need not make the `traditional
-approximation'. To be able to support consistent non-hydrostatic forms the
-shallow atmosphere approximation can be relaxed - when dividing through by $
-r $ in, for example, (\ref{eq:gu-speherical}), we do not replace $r$ by $a$,
-the radius of the earth.
+Most models are based on the `hydrostatic primitive equations' (HPE's)
+in which the vertical momentum equation is reduced to a statement of
+hydrostatic balance and the `traditional approximation' is made in
+which the Coriolis force is treated approximately and the shallow
+atmosphere approximation is made.  MITgcm need not make the
+`traditional approximation'. To be able to support consistent
+non-hydrostatic forms the shallow atmosphere approximation can be
+relaxed - when dividing through by $ r $ in, for example,
+(\ref{eq:gu-speherical}), we do not replace $r$ by $a$, the radius of
+the earth.
 
 \subsubsection{Hydrostatic and quasi-hydrostatic forms}
 \label{sec:hydrostatic_and_quasi-hydrostatic_forms}
@@ -815,7 +816,7 @@
 
 \subsubsection{Non-hydrostatic and quasi-nonhydrostatic forms}
 
-The MIT model presently supports a full non-hydrostatic ocean isomorph, but
+MITgcm presently supports a full non-hydrostatic ocean isomorph, but
 only a quasi-non-hydrostatic atmospheric isomorph.
 
 \paragraph{Non-hydrostatic Ocean}
@@ -1123,7 +1124,7 @@
 Tangent linear and adjoint counterparts of the forward model are described
 in Chapter 5.
 
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.22 2004/10/17 04:15:13 jmc Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.24 2006/04/05 02:27:32 edhill Exp $
 % $Name:  $
 
 \section{Appendix ATMOSPHERE}
@@ -1252,7 +1253,7 @@
 \frac{D\theta }{Dt} &=&\frac{\mathcal{Q}}{\Pi } 
 \end{eqnarray}
 
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.22 2004/10/17 04:15:13 jmc Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.24 2006/04/05 02:27:32 edhill Exp $
 % $Name:  $
 
 \section{Appendix OCEAN}
@@ -1469,7 +1470,7 @@
 _{nh}=0$ form of these equations that are used throughout the ocean modeling
 community and referred to as the primitive equations (HPE).
 
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.22 2004/10/17 04:15:13 jmc Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.24 2006/04/05 02:27:32 edhill Exp $
 % $Name:  $
 
 \section{Appendix:OPERATORS}