[cig-commits] r8982 - geodyn/3D/MAG/trunk/doc
sue at geodynamics.org
sue at geodynamics.org
Thu Jan 3 14:08:39 PST 2008
Author: sue
Date: 2008-01-03 14:08:37 -0800 (Thu, 03 Jan 2008)
New Revision: 8982
Modified:
geodyn/3D/MAG/trunk/doc/mag_book.lyx
geodyn/3D/MAG/trunk/doc/mag_book.pdf
Log:
disclaimer required by nsf added
Modified: geodyn/3D/MAG/trunk/doc/mag_book.lyx
===================================================================
--- geodyn/3D/MAG/trunk/doc/mag_book.lyx 2008-01-03 21:49:12 UTC (rev 8981)
+++ geodyn/3D/MAG/trunk/doc/mag_book.lyx 2008-01-03 22:08:37 UTC (rev 8982)
@@ -1,5 +1,5 @@
-#LyX 1.4.3 created this file. For more info see http://www.lyx.org/
-\lyxformat 245
+#LyX 1.5.1 created this file. For more info see http://www.lyx.org/
+\lyxformat 276
\begin_document
\begin_header
\textclass book
@@ -12,13 +12,21 @@
\end_preamble
\language english
\inputencoding auto
-\fontscheme default
+\font_roman default
+\font_sans default
+\font_typewriter default
+\font_default_family default
+\font_sc false
+\font_osf false
+\font_sf_scale 100
+\font_tt_scale 100
\graphics default
\paperfontsize default
\spacing single
\papersize default
\use_geometry true
\use_amsmath 0
+\use_esint 0
\cite_engine basic
\use_bibtopic false
\paperorientation portrait
@@ -35,7 +43,8 @@
\papersides 2
\paperpagestyle headings
\tracking_changes false
-\output_changes true
+\output_changes false
+\author ""
\end_header
\begin_body
@@ -87,7 +96,7 @@
\end_layout
\begin_layout Author
-© California Institute of Technology
+© California Institute of Technology
\newline
Peter Olson and Wei Mi
\newline
@@ -112,7 +121,7 @@
\begin_layout Standard
\noindent
-\begin_inset LatexCommand \tableofcontents{}
+\begin_inset LatexCommand tableofcontents
\end_inset
@@ -169,18 +178,24 @@
\begin_layout Standard
The style of this publication is based on the
-\begin_inset LatexCommand \htmlurl[Apple Publications Style Guide]{developer.apple.com/documentation/UserExperience/Conceptual/APStyleGuide/AppleStyleGuide2003.pdf}
+\begin_inset LatexCommand htmlurl
+name "Apple Publications Style Guide"
+target "developer.apple.com/documentation/UserExperience/Conceptual/APStyleGuide/AppleStyleGuide2003.pdf"
\end_inset
, as recommended by
-\begin_inset LatexCommand \htmlurl[Python.org]{www.python.org}
+\begin_inset LatexCommand htmlurl
+name "Python.org"
+target "www.python.org"
\end_inset
.
The documentation was produced using
-\begin_inset LatexCommand \htmlurl[LyX]{www.lyx.org}
+\begin_inset LatexCommand htmlurl
+name "LyX"
+target "www.lyx.org"
\end_inset
@@ -192,7 +207,9 @@
\begin_layout Standard
Errors and bug fixes in this manual should be directed to the
-\begin_inset LatexCommand \url[CIG Geodynamo Mailing List]{cig-geodyn at geodynamics.org}
+\begin_inset LatexCommand url
+name "CIG Geodynamo Mailing List"
+target "cig-geodyn at geodynamics.org"
\end_inset
@@ -244,29 +261,27 @@
Geophys.
Astrophys.
Fluid Dyn.,
-\series bold
\emph default
-\series default
\emph on
70
\series bold
-,
+,
\series default
\emph default
-113-136.
+ 113-136.
\end_layout
\begin_layout Itemize
Olson, P., G.A.
Glatzmaier (1995), Magnetoconvection in a rotating spherical shell: structure
of flow in the outer core.
-
+
\emph on
- Phys.
- Earth Planet Int., 92,
+Phys.
+ Earth Planet Int., 92,
\emph default
-109-118.
+ 109-118.
\end_layout
\begin_layout Itemize
@@ -329,9 +344,9 @@
\begin_layout Itemize
Christensen, et al.
(2001), A numerical dynamo benchmark.
-
+
\emph on
- Phys.
+Phys.
Earth Planet Int., 128
\emph default
, 25-34 (benchmark cases).
@@ -344,7 +359,9 @@
Glatzmaier, U.
Christensen, P.
Olson), and
-\begin_inset LatexCommand \htmlurl[CIG]{geodynamics.org}
+\begin_inset LatexCommand htmlurl
+name "CIG"
+target "geodynamics.org"
\end_inset
@@ -357,7 +374,12 @@
\begin_layout Standard
MAG development was funded by grants from NASA HPC and NSF Geophysics.
- Continued support of MAG is made possible under NSF EAR-0406751.
+ Continued support of MAG is based upon work supported by the National Science
+ Foundation under Grant No.
+ EAR-0406751.
+ Any opinions, findings, and conclusions or recommendations expressed in
+ this material are those of the authors and do not necessarily reflect the
+ views of the National Science Foundation.
\end_layout
\begin_layout Part
@@ -406,7 +428,8 @@
\begin_layout Standard
All variables are non-dimensional (see Appendix
-\begin_inset LatexCommand \ref{cha:Variables-used-in}
+\begin_inset LatexCommand ref
+reference "cha:Variables-used-in"
\end_inset
@@ -426,12 +449,14 @@
\begin_layout Standard
Additional technical information is found in
-\begin_inset LatexCommand \cite{key-1}
+\begin_inset LatexCommand cite
+key "key-1"
\end_inset
-
-\begin_inset LatexCommand \cite{key-8}
+\begin_inset LatexCommand cite
+key "key-8"
\end_inset
@@ -447,7 +472,8 @@
equations for dynamo action due to thermal convection of an electrically
conducting fluid in a rotating spherical shell (e.g., Olson et al.
1999)
-\begin_inset LatexCommand \cite{key-5}
+\begin_inset LatexCommand cite
+key "key-5"
\end_inset
@@ -530,12 +556,14 @@
\begin_layout Standard
Four basic non-dimensional parameters in
-\begin_inset LatexCommand \ref{eq:1}
+\begin_inset LatexCommand ref
+reference "eq:1"
\end_inset
-
-\begin_inset LatexCommand \ref{eq:4}
+\begin_inset LatexCommand ref
+reference "eq:4"
\end_inset
@@ -654,7 +682,9 @@
tar
\family default
file) from the
-\begin_inset LatexCommand \htmlurl[Geodynamics Software Packages web page]{geodynamics.org/cig/software/packages}
+\begin_inset LatexCommand htmlurl
+name "Geodynamics Software Packages web page"
+target "geodynamics.org/cig/software/packages"
\end_inset
@@ -673,7 +703,8 @@
the latest MAG source code directly from the CIG source code repository,
instead of using the prepared source package.
See Section
-\begin_inset LatexCommand \ref{sec:Software-Repository}
+\begin_inset LatexCommand ref
+reference "sec:Software-Repository"
\end_inset
@@ -687,13 +718,17 @@
\begin_layout Standard
For help, send e-mail to the
-\begin_inset LatexCommand \url[CIG Geodynamo Mailing List]{cig-geodyn at geodynamics.org}
+\begin_inset LatexCommand url
+name "CIG Geodynamo Mailing List"
+target "cig-geodyn at geodynamics.org"
\end_inset
.
You can subscribe to the Mailing List and view archived discussion at
-\begin_inset LatexCommand \htmlurl[Geodynamics Mail Lists]{geodynamics.org/cig/lists}
+\begin_inset LatexCommand htmlurl
+name "Geodynamics Mail Lists"
+target "geodynamics.org/cig/lists"
\end_inset
@@ -714,7 +749,9 @@
\begin_layout Itemize
For Windows you need to install
-\begin_inset LatexCommand \htmlurl[cygwin]{cygwin.com}
+\begin_inset LatexCommand htmlurl
+name "cygwin"
+target "cygwin.com"
\end_inset
@@ -731,7 +768,9 @@
\begin_layout Standard
Download MAG from the
-\begin_inset LatexCommand \htmlurl[Geodynamics website]{geodynamics.org}
+\begin_inset LatexCommand htmlurl
+name "Geodynamics website"
+target "geodynamics.org"
\end_inset
@@ -762,7 +801,8 @@
\end_layout
\begin_layout Subsection
-\begin_inset LatexCommand \label{sub:MAG-file-structure}
+\begin_inset LatexCommand label
+name "sub:MAG-file-structure"
\end_inset
@@ -818,7 +858,8 @@
conductive temperature perturbation with imposed perturbation with l=4,
m=4, and running for a short time.
This is the ``benchmark0'' test case in Christensen et al., 2001
-\begin_inset LatexCommand \cite{benchmark cases}
+\begin_inset LatexCommand cite
+key "benchmark cases"
\end_inset
@@ -831,7 +872,8 @@
\size default
, the dynamo ``benchmark1'' case in Christensen et al.
-\begin_inset LatexCommand \cite{benchmark cases}
+\begin_inset LatexCommand cite
+key "benchmark cases"
\end_inset
@@ -878,7 +920,8 @@
\size default
obtained with short runs of benchmark0 and benchmark1 on a Linux workstation.
Explanations of the contents of these files are found in Appendix
-\begin_inset LatexCommand \ref{cha:MAG-Output-File}
+\begin_inset LatexCommand ref
+reference "cha:MAG-Output-File"
\end_inset
@@ -906,7 +949,8 @@
\end_layout
\begin_layout Subsection
-\begin_inset LatexCommand \label{sub:Prepare-MAG-for}
+\begin_inset LatexCommand label
+name "sub:Prepare-MAG-for"
\end_inset
@@ -937,8 +981,9 @@
in the source directory, which by default uses the existing
\family typewriter
\size small
-param.f
+param.f
\family default
+
\size default
grid and symmetry
\end_layout
@@ -990,7 +1035,8 @@
\end_deeper
\begin_layout Section
-\begin_inset LatexCommand \label{sec:Software-Repository}
+\begin_inset LatexCommand label
+name "sec:Software-Repository"
\end_inset
@@ -999,7 +1045,9 @@
\begin_layout Standard
The MAG source code is available via a Subversion server at the
-\begin_inset LatexCommand \htmlurl[Geodynamics website]{geodynamics.org}
+\begin_inset LatexCommand htmlurl
+name "Geodynamics website"
+target "geodynamics.org"
\end_inset
@@ -1011,9 +1059,10 @@
\begin_layout Quote
\series bold
-NOTE:
+NOTE:
\series default
-If you are content with the prepared source package, you may skip this section.
+ If you are content with the prepared source package, you may skip this
+ section.
\end_layout
\begin_layout Subsection
@@ -1039,7 +1088,9 @@
\begin_layout Standard
It should return a usage message.
For more information on Subversion, visit the
-\begin_inset LatexCommand \htmlurl[Subversion website]{subversion.tigris.org}
+\begin_inset LatexCommand htmlurl
+name "Subversion website"
+target "subversion.tigris.org"
\end_inset
@@ -1076,7 +1127,8 @@
\end_inset
is the directory created with the file structure mentioned in
-\begin_inset LatexCommand \ref{sub:MAG-file-structure}
+\begin_inset LatexCommand ref
+reference "sub:MAG-file-structure"
\end_inset
@@ -1097,7 +1149,8 @@
\begin_layout Enumerate
Uncompress all files, and create a path (see
-\begin_inset LatexCommand \ref{sub:Prepare-MAG-for}
+\begin_inset LatexCommand ref
+reference "sub:Prepare-MAG-for"
\end_inset
@@ -1133,8 +1186,9 @@
Examples of
\family typewriter
\size small
-param.f
+param.f
\family default
+
\size default
are
\family typewriter
@@ -1258,15 +1312,16 @@
\family typewriter
\size default
-ls.bench0, g[i].bench0
+ls.bench0, g[i].bench0
\family default
-and
+ and
\family typewriter
d[i].bench0
\family default
, where i=0,1,2...9.
See Appendix
-\begin_inset LatexCommand \ref{cha:MAG-Output-File}
+\begin_inset LatexCommand ref
+reference "cha:MAG-Output-File"
\end_inset
@@ -1315,7 +1370,8 @@
\end_layout
\begin_layout Chapter
-\begin_inset LatexCommand \label{cha:Postprocessing-and-Graphics}
+\begin_inset LatexCommand label
+name "cha:Postprocessing-and-Graphics"
\end_inset
@@ -1339,13 +1395,17 @@
\family default
is the directory under which you installed MAG.
We should mention here that IDL is a commercial visualization tool by
-\begin_inset LatexCommand \htmlurl[ITT Visual Information Solutions]{www.ittvis.com/idl}
+\begin_inset LatexCommand htmlurl
+name "ITT Visual Information Solutions"
+target "www.ittvis.com/idl"
\end_inset
.
A free IDL compatible program called
-\begin_inset LatexCommand \htmlurl[GDL]{gnudatalanguage.sourceforge.net}
+\begin_inset LatexCommand htmlurl
+name "GDL"
+target "gnudatalanguage.sourceforge.net"
\end_inset
@@ -1379,7 +1439,8 @@
statistics.
This version reads an l-file consisting of 17 time series, the first record
being dimensionless time (see Appendix
-\begin_inset LatexCommand \ref{cha:MAG-Output-File}
+\begin_inset LatexCommand ref
+reference "cha:MAG-Output-File"
\end_inset
@@ -1387,12 +1448,14 @@
Energies and rms magnetic field and velocity are scaled as in MAG; tilt
is dipole vector colatitude; pole longitude is dipole vector longitude.
Figures
-\begin_inset LatexCommand \ref{fig:Time-series-plot}
+\begin_inset LatexCommand ref
+reference "fig:Time-series-plot"
\end_inset
and
-\begin_inset LatexCommand \ref{fig:Spectra-plot-of}
+\begin_inset LatexCommand ref
+reference "fig:Spectra-plot-of"
\end_inset
@@ -1423,9 +1486,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:Time-series-plot}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:Time-series-plot"
+
\end_inset
Time series plot of energy
@@ -1436,6 +1503,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Standard
\noindent
\align center
@@ -1457,9 +1529,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:Spectra-plot-of}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:Spectra-plot-of"
+
\end_inset
Spectra plot of a time depentant dynamo
@@ -1470,6 +1546,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Section
Interactive IDL Procedures
\end_layout
@@ -1502,7 +1583,8 @@
Producing each plot is straightforward and accomplished by choosing from
the option menu.
Figure
-\begin_inset LatexCommand \ref{fig:IDL-figure-with}
+\begin_inset LatexCommand ref
+reference "fig:IDL-figure-with"
\end_inset
@@ -1532,9 +1614,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:IDL-figure-with}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:IDL-figure-with"
+
\end_inset
IDL figure with Map option
@@ -1545,6 +1631,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Standard
MAGVOL.pro is another interactive IDL procedure to display volume results
from rotating convection, magnetoconvection and dynamo calculations (written
@@ -1583,7 +1674,8 @@
the z-component of vorticity, kinetic and magnetic energy, joule heating,
work by Lorentz forces and buoyancy forces.
Figure
-\begin_inset LatexCommand \ref{fig:Kinetic-energy-(yellow)}
+\begin_inset LatexCommand ref
+reference "fig:Kinetic-energy-(yellow)"
\end_inset
@@ -1616,9 +1708,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:Kinetic-energy-(yellow)}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:Kinetic-energy-(yellow)"
+
\end_inset
Kinetic energy (yellow) and Magnetic energy (blue) plot by the MAGVOL procedure
@@ -1629,6 +1725,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Chapter
Examples
\end_layout
@@ -1647,7 +1748,8 @@
Historically, these are the cases defined in the benchmark study published
in the 2001 paper by Christensen et al.
-\begin_inset LatexCommand \cite{benchmark cases}
+\begin_inset LatexCommand cite
+key "benchmark cases"
\end_inset
@@ -1682,7 +1784,8 @@
.
Note that the definition of the Rayleigh number differs from the one in
the published cases
-\begin_inset LatexCommand \cite{benchmark cases}
+\begin_inset LatexCommand cite
+key "benchmark cases"
\end_inset
@@ -1695,7 +1798,8 @@
\end_inset
.
-\begin_inset LatexCommand \cite{benchmark cases}
+\begin_inset LatexCommand cite
+key "benchmark cases"
\end_inset
@@ -2229,7 +2333,8 @@
\begin_layout Standard
This case has run on 32-bit and 64-bit Intel processors.
Figure
-\begin_inset LatexCommand \ref{fig:Field-Plot1}
+\begin_inset LatexCommand ref
+reference "fig:Field-Plot1"
\end_inset
@@ -2237,14 +2342,16 @@
dipole and the dipole tilt on the outer boundary.
It indicated a magnetic field reversal between time steps 25 and 30.
Figure
-\begin_inset LatexCommand \ref{fig:Field-Plot2}
+\begin_inset LatexCommand ref
+reference "fig:Field-Plot2"
\end_inset
shows a longer run of MAG, where we see the magnetic field reversed again.
At this time, the magnetic field had weakened substantially.
In Figure
-\begin_inset LatexCommand \ref{fig:The-pole}
+\begin_inset LatexCommand ref
+reference "fig:The-pole"
\end_inset
@@ -2275,9 +2382,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:Field-Plot1}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:Field-Plot1"
+
\end_inset
Field Plot for Reversal Dynamo Case
@@ -2288,6 +2399,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Standard
\noindent
\align center
@@ -2310,9 +2426,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:Field-Plot2}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:Field-Plot2"
+
\end_inset
Field Plot for Reversal Dynamo Case (longer run)
@@ -2323,6 +2443,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Standard
\noindent
\align center
@@ -2359,9 +2484,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:The-pole}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:The-pole"
+
\end_inset
Magnetic Field Pole Plot.
@@ -2374,6 +2503,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Subsection
Creating a Reversal Dynamo Movie
\end_layout
@@ -2410,7 +2544,8 @@
For our reversal dynamo case we examine the field plot and decide to record
the first field reversal.
As shown the figure
-\begin_inset LatexCommand \ref{fig:Interval-to-record}
+\begin_inset LatexCommand ref
+reference "fig:Interval-to-record"
\end_inset
@@ -2462,7 +2597,8 @@
and displays the magnetic field at the outer surface.
This procedure can also create JPG files of the movie-frame images.
Figure
-\begin_inset LatexCommand \ref{fig:a:-first-frame}
+\begin_inset LatexCommand ref
+reference "fig:a:-first-frame"
\end_inset
@@ -2492,9 +2628,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:Interval-to-record}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:Interval-to-record"
+
\end_inset
Interval to record movie
@@ -2505,6 +2645,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Standard
\noindent
\align center
@@ -2537,9 +2682,13 @@
\end_layout
-\begin_layout Caption
-\begin_inset LatexCommand \label{fig:a:-first-frame}
+\begin_layout Standard
+\begin_inset Caption
+\begin_layout Standard
+\begin_inset LatexCommand label
+name "fig:a:-first-frame"
+
\end_inset
Reversal Dynamo Movie.
@@ -2551,6 +2700,11 @@
\end_layout
+\end_inset
+
+
+\end_layout
+
\begin_layout Subsubsection
Creating MPEGs with IDL
\end_layout
@@ -2559,7 +2713,9 @@
IDL provides an IDLgrMPEG class that allows the user to save an array of
image frames as an MPEG movie.
See the
-\begin_inset LatexCommand \htmlurl[IDL Reference Guide]{www.rsinc.com/idl/pdfs/refguide.pdf}
+\begin_inset LatexCommand htmlurl
+name "IDL Reference Guide"
+target "www.rsinc.com/idl/pdfs/refguide.pdf"
\end_inset
@@ -2775,7 +2931,8 @@
In contrast, the geomagnetism scientific community uses real-valued Schmidt-typ
e spherical harmonics for representing the main field, with dimensional
coefficients called the Gauss coefficients (see
-\begin_inset LatexCommand \cite{key-8,key-9}
+\begin_inset LatexCommand cite
+key "key-8,key-9"
\end_inset
@@ -2818,7 +2975,8 @@
\begin_layout Chapter
\start_of_appendix
-\begin_inset LatexCommand \label{cha:Variables-used-in}
+\begin_inset LatexCommand label
+name "cha:Variables-used-in"
\end_inset
@@ -4315,7 +4473,8 @@
\end_layout
\begin_layout Chapter
-\begin_inset LatexCommand \label{cha:MAG-Input-File}
+\begin_inset LatexCommand label
+name "cha:MAG-Input-File"
\end_inset
@@ -4722,7 +4881,8 @@
\end_layout
\begin_layout Chapter
-\begin_inset LatexCommand \label{cha:MAG-Output-File}
+\begin_inset LatexCommand label
+name "cha:MAG-Output-File"
\end_inset
@@ -4805,9 +4965,9 @@
\begin_layout Quote
\series bold
-Note:
+Note:
\series default
-If one of the above files already exists, the program will not run.
+ If one of the above files already exists, the program will not run.
\end_layout
\begin_layout Standard
@@ -5719,8 +5879,12 @@
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "1"
+key "key-1"
-\bibitem [1]{key-1}
+\end_inset
+
Olson, P., G.A.
Glatzmaier (1995), Highly supercritical thermal convection in a rotating
spherical shell: centrifugal vs.
@@ -5730,36 +5894,42 @@
Geophys.
Astrophys.
Fluid Dyn.,
-\series bold
\emph default
-\series default
\emph on
70
\series bold
-,
+,
\series default
\emph default
-113-136
+ 113-136
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "2"
+key "key-2"
-\bibitem [2]{key-2}
+\end_inset
+
Olson, P., G.A.
Glatzmaier (1995), Magnetoconvection in a rotating spherical shell: structure
of flow in the outer core.
-
+
\emph on
- Phys.
- Earth Planet Int., 92,
+Phys.
+ Earth Planet Int., 92,
\emph default
-109-118
+ 109-118
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "3"
+key "key-3"
-\bibitem [3]{key-3}
+\end_inset
+
Olson, P., G.A.
Glatzmaier (1996), Magnetoconvection and Thermal Coupling of the Earth's
Core and Mantle.
@@ -5775,8 +5945,12 @@
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "4"
+key "key-4"
-\bibitem [4]{key-4}
+\end_inset
+
Olson, P., U.
Christensen, G.A.
Glatzmaier (1999), Numerical Modeling of the Geodynamo: Mechanisms of Field
@@ -5791,8 +5965,12 @@
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "5"
+key "key-5"
-\bibitem [5]{key-5}
+\end_inset
+
Christensen, U., P.
Olson, G.A.
Glatzmaier (1999), Numerical modelling of the geodynamo: a systematic parameter
@@ -5807,21 +5985,29 @@
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "6"
+key "benchmark cases"
-\bibitem [6]{benchmark cases}
+\end_inset
+
Christensen, et al.
(2001), A numerical dynamo benchmark.
-
+
\emph on
- Phys.
+Phys.
Earth Planet Int., 128
\emph default
, 25-34 (benchmark cases)
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "7"
+key "key-7"
-\bibitem [7]{key-7}
+\end_inset
+
Olson, P., G.A.
Glatzmaier (2005), Probing the geodynamo.
@@ -5830,14 +6016,18 @@
\emph default
(2)
\emph on
-,
+,
\emph default
-29-35
+ 29-35
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+label "8"
+key "key-8"
-\bibitem [8]{key-8}
+\end_inset
+
Christensen, U.R., J.
Aubert (2006), Scaling properties of convection-driven dynamos in rotating
spherical shells and application to planetary magnetic fields.
@@ -5852,8 +6042,11 @@
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+key "key-9"
-\bibitem {key-9}
+\end_inset
+
Backus, G., Parker, R., Constable, C.
\emph on
@@ -5863,11 +6056,14 @@
\end_layout
\begin_layout Bibliography
+\begin_inset LatexCommand bibitem
+key "key-10"
-\bibitem {key-10}
- Merrill, R.T., McElhinny, M.W., McFadden, P.L.,
+\end_inset
+
+ Merrill, R.T., McElhinny, M.W., McFadden, P.L.,
\emph on
- The Magnetic Field of the Earth, Paleomagnetism, the Core, and the Deep
+The Magnetic Field of the Earth, Paleomagnetism, the Core, and the Deep
Mantle
\emph default
, Academic Press, 1998
Modified: geodyn/3D/MAG/trunk/doc/mag_book.pdf
===================================================================
(Binary files differ)
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