Georg Baum wrote:
See attached.
Thanks :)
<>
This should not happen, because lyx should select the correct babel options.
Can you send a minimal example file showing this behaviour?
If the pasted text is not really in a foreign language, mark it and then
reset the language in Format->Character.
Ah, thanks. Resetting the language works. I'm attaching two files anyway in case someone wants to debug the problem further. Try pasting something from chapter 5 to chapter 6 and try a DVI view to see the problem. (using LyX 1.3.3-win32)
(Herbert: thanks for the appendix numbering code)
- Henrik
#LyX 1.3 created this file. For more info see http://www.lyx.org/ \lyxformat 221 \textclass mythesis \begin_preamble
%%%%%%%%% REF MACROS %%%%%%%%
\def\apj{ApJ}
\def\mnras{MNRAS}
\def\apjl{ApJL}
\def\aap{A\&A}
%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%% LAYOUT %%%%%%%%%%
\raggedbottom
\end_preamble
\language british
\inputencoding auto
\fontscheme default
\graphics default
\paperfontsize 12
\spacing other 1.50
\papersize a4paper
\paperpackage a4
\use_geometry 1
\use_amsmath 0
\use_natbib 1
\use_numerical_citations 0
\paperorientation portrait
\leftmargin 1.25in
\topmargin 1.6in
\rightmargin 0.8in
\bottommargin 1in
\headsep 0.6in
\secnumdepth 3
\tocdepth 3
\paragraph_separation indent
\defskip medskip
\quotes_language english
\quotes_times 2
\papercolumns 1
\papersides 1
\paperpagestyle uheadings
\layout Chapter
Results, part I
\layout Standard
This chapter is a first look at the experimental results starting with a
description of the raw data generated by the simulations and the data reduction
and analysis routines used to extract useful scientific information.
We also examine the first stage of the simulation, the cooling phase during
the first 300 Myrs, which is identical for all simulations.
\layout Section
The raw data
\layout Standard
\noun on
Enzo
\noun default
stores the main grid data in industry standard NCSA Hierarchical Data Format
(HDF)
\begin_inset Foot
collapsed true
\layout Standard
See
\family typewriter
http://hdf.ncsa.uiuc.edu
\family default
for details.
\end_inset
.
These files contain the 11? variables listed in table X, and some meta
data, such as variable names.
The HDF format is valuable because the date can be read directly by standard
visualisation programs like HDFLook and IDL
\begin_inset Foot
collapsed true
\layout Standard
See:
\family typewriter
http://daac.gsfc.nasa.gov/MODIS/HDFLook/
\family default
and
\family typewriter
http://www.rsinc.com/idl/
\family default
.
\end_inset
.
The raw data can therefore be studied directly as the simulation progresses
to ensure that it develops as expected.
However, each grid in the grid structure is stored in a separate HDF file,
and with several thousand such grids it is impractrical to analyse this
data directly.
Viewing any one grid file only gives a low resolution view of the domain
or a high resolution view of a very small region.
To be scientifically useful, the data is reduced in a number of ways.
Enzo includes as standard data reduction routines for producing 3-dimensional
extractions, 2-dimensional projections, and 1-dimensional vectors averaged
over radial shells.
A fourth reduction tool was developed during this project to extract an
arbitrary set of point samples from the domain.
\the_end
#LyX 1.3 created this file. For more info see http://www.lyx.org/ \lyxformat 221 \textclass mythesis2 \begin_preamble %%%%%%%%% REF MACROS %%%%%%%% \def\apj{ApJ} \def\mnras{MNRAS} \def\apjl{ApJL} %%%%%%%%%%%%%%%%%%%%%%%% \end_preamble \language english \inputencoding auto \fontscheme default \graphics default \paperfontsize default \spacing onehalf \papersize a4paper \paperpackage widemarginsa4 \use_geometry 0 \use_amsmath 0 \use_natbib 1 \use_numerical_citations 0 \paperorientation portrait \secnumdepth 3 \tocdepth 3 \paragraph_separation indent \defskip medskip \quotes_language english \quotes_times 2 \papercolumns 1 \papersides 1 \paperpagestyle default \layout Chapter Discussion \layout Section Previous simulations \layout Standard Churazov etal. \begin_inset LatexCommand \cite{Churazov_etal_2001} \end_inset performed the first significant numerical bubble experiment in 2000. The setup was modeled on the M87 galaxy and its surroundings, based on ROSAT data by Nulsen and Böhringer \begin_inset LatexCommand \cite{Nulsen&Bohringer_1995} \end_inset , with typical densities of 0.02 \begin_inset Formula $\textrm{cm}^{-3}$ \end_inset and temperatures of 2 keV. The simulations were 2-dimensional with medium resolution at \begin_inset Formula $200^{2}$ \end_inset cells, and rotational symetry was chosen about an axis parallel with the gravitational force. The computational domain was limited, reaching out 51kpc from the cluster core. A 2-dimensional gravitational potential and temperature profile were selected, and a corresponding density gradient was constructed in hydrostatic equlibrium. A sperical heated bubble with a 5 kpc radius was created at 9 kpc from the core and alowed to rise in the gravitational potential. The bubble was created by instantaneously replacing the ambient gas with material at 100 times the original temperature and 0.01 times the original density, thus maintaining pressure equilibrium. The simulations were naturally limited to the time it took the bubble to cross the computational domain, which in this case was 50-70Myrs. The authors argued that this short time scale meant that radiative cooling was not important, and therefore was not applied. \the_end
