--- manual/s_overview/text/manual.tex	2001/10/25 15:24:01	1.8
+++ manual/s_overview/text/manual.tex	2001/11/13 20:13:07	1.9
@@ -1,4 +1,4 @@
-% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.8 2001/10/25 15:24:01 cnh Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.9 2001/11/13 20:13:07 adcroft 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 1.8 2001/10/25 15:24:01 cnh Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.9 2001/11/13 20:13:07 adcroft Exp $
 % $Name:  $
 
 \section{Introduction}
@@ -89,7 +89,7 @@
 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 1.8 2001/10/25 15:24:01 cnh Exp $
+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.9 2001/11/13 20:13:07 adcroft Exp $
 % $Name:  $
 
 \section{Illustrations of the model in action}
@@ -191,7 +191,7 @@
 ocean may be influenced by rotation when the deformation radius is smaller
 than the width of the cooling region. Rather than gravity plumes, the
 mechanism for moving dense fluid down the shelf is then through geostrophic
-eddies. The simulation shown in the figure \ref{fig::convect-and-topo}
+eddies. The simulation shown in the figure \ref{fig:convect-and-topo}
 (blue is cold dense fluid, red is
 warmer, lighter fluid) employs the non-hydrostatic capability of MITgcm to
 trigger convection by surface cooling. The cold, dense water falls down the
@@ -289,7 +289,7 @@
 \input{part1/lab_figure}
 %%CNHend
 
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+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.9 2001/11/13 20:13:07 adcroft Exp $
 % $Name:  $
 
 \section{Continuous equations in `r' coordinates}
@@ -351,7 +351,7 @@
 
 \begin{equation}
 \frac{DS}{Dt}=\mathcal{Q}_{S}\text{ humidity/salinity}
-\label{eq:humidtity_salt}
+\label{eq:humidity_salt}
 \end{equation}
 
 Here:
@@ -525,7 +525,7 @@
 atmosphere)}  \label{eq:moving-bc-atmos}
 \end{eqnarray}
 
-Then the (hydrostatic form of) equations (\ref{eq:horizontal_mtm}-\ref{eq:humidity_slainty}) 
+Then the (hydrostatic form of) equations (\ref{eq:horizontal_mtm}-\ref{eq:humidity_salt}) 
 yields a consistent set of atmospheric equations which, for convenience, are written out in $p$
 coordinates in Appendix Atmosphere - see eqs(\ref{eq:atmos-prime}).
 
@@ -562,7 +562,7 @@
 \end{eqnarray}
 where $\eta $ is the elevation of the free surface.
 
-Then equations (\ref{eq:horizontal_mtm}-\ref{eq:humidity_slainty}) yield a consistent set 
+Then equations (\ref{eq:horizontal_mtm}-\ref{eq:humidity_salt}) yield a consistent set 
 of oceanic equations
 which, for convenience, are written out in $z$ coordinates in Appendix Ocean
 - see eqs(\ref{eq:ocean-mom}) to (\ref{eq:ocean-salt}).
@@ -1028,7 +1028,7 @@
 Tangent linear and adjoint counterparts of the forward model are described
 in Chapter 5.
 
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+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.9 2001/11/13 20:13:07 adcroft Exp $
 % $Name:  $
 
 \section{Appendix ATMOSPHERE}
@@ -1155,7 +1155,7 @@
 \frac{D\theta }{Dt} &=&\frac{\mathcal{Q}}{\Pi } 
 \end{eqnarray}
 
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+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.9 2001/11/13 20:13:07 adcroft Exp $
 % $Name:  $
 
 \section{Appendix OCEAN}
@@ -1371,7 +1371,7 @@
 _{nh}=0$ form of these equations that are used throughout the ocean modeling
 community and referred to as the primitive equations (HPE).
 
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+% $Header: /home/ubuntu/mnt/e9_copy/manual/s_overview/text/manual.tex,v 1.9 2001/11/13 20:13:07 adcroft Exp $
 % $Name:  $
 
 \section{Appendix:OPERATORS}
