%% file: rjr-asp-example.tex = Rob Rutten LaTeX+BibTeX example for ASP-CS
%% init: Mar  9 2007 
%% last: Mar 23 2007 
%% note: %RR = Rob Rutten comment
%%       see http://www.astro.uu.nl/~rutten/rr/tex/manuals/publishers/aspcs/rjr-recipes/authors/Readme-author.txt 


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\documentclass[11pt,twoside]{article}
\usepackage{rjr-asp}
\usepackage{lscape}
\usepackage{epsfig,graphicx,natbib,url}  %RR additions
%%\usepackage{hyperref} %RR possible adddition
\pagestyle{myheadings}

\def\figspath{.}  %RR to be redefined by editor at insertion into book 

\hyphenation{Krij-ger Schrij-ver}


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\begin{document}

\markboth{R.J. Rutten et al.}{Nature of the Solar Chromosphere}
\title{On the Nature of the Solar Chromosphere}  
\author{Robert J. Rutten$^{1,2}$, 
        Alfred G. de Wijn$^1$  %RR no , after the next to last name
        and 
        Jorrit Leenaarts$^1$}
\affil{$^1$Sterrekundig Instituut, Utrecht University, The Netherlands \\
       $^2$Institutt for Teoretisk Astrofysikk, University of Oslo, Norway}
  
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\begin{abstract} 
  Sloppy authors do not read section ``Latex do's and don't's'' in
  file {\tt Readme-author.txt} at
  \url{http://www.astro.uu.nl/~rutten/rr/tex/manuals/publishers/aspcs/rjr-recipes/authors}.
  Sloppy authors also add postal addresses above, wrongly use "......"
  instead of ``......'', do not add space-making backslashes after et
  al., \AA, etc., do not use tildes for non-breakable spaces before
  units and after initials, do not set units in roman font, do not set
  the e of electron in roman, do not use bibtex but muck around with
  error-prone self-made bibitem entries, do not use a spell checker
  (set it to American), do not use the url command for websites.
  French authors (usually most sloppy) use ``eventually'' wrongly.

  The abstract is set in small type so that you can write it very
  long, useful when potential readers look it up in ADS.  Then split
  it in paragraphs as done here.
\end{abstract}
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\section{Introduction}      \label{rutten-sec:introduction}
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Movies from the Dutch Open Telescope\footnote{All DOT
% 
  data are public and available under {\em DOT database\/} at
  \url{http://dot.astro.uu.nl}.  The movie sampled here in
  Fig.~\ref{rutten-fig:limb} resides there also, under {\em DOT
  movies}.}
%
  (\cite{2004A&A...413.1183R}) % Rutten++ DOT tomo1 
%
suggest that much so-called chromosphere is actually transition
region, that much other so-called chromosphere is actually upper
photosphere, and that only those \Halpha\ mottles and fibrils that
span across and between internetwork cells and active regions
constitute the actual chromosphere.  This is argued in a paper by the
first author in the Sac Peak ``Steinfest'' proceedings from which this
example was prepared through cutting out most of the text -- while
adding two co-authors to show how to do that.  More should have been
taken out because the remaining text overflows on the third page.  ASP
proceedings articles start on righthand pages, so that each paper
should fill an even number of pages.  This fixed format enables you to
place corresponding text and figures on adjacent odd-even pages,
simultaneously in view both in the book and in pdf printouts.

%RR figure always between blank lines
%============================================================================
\begin{figure}  %RR no location specifier
  \centering
  \includegraphics[width=\textwidth]{\figspath/rutten-limb}
  \caption[]{\label{rutten-fig:limb}  %RR don't forget the [] 
%
  Three partial near-limb images.  Ticks at arcsec intervals.  The
  limb is just above the top.  {\em Left\/}: G band.  {\em Center\/}:
  \CaIIH\ wing.  {\em Right\/}: \CaIIH\ line center.  The reader is
  invited to zoom in on the line-center ``straws'' with a pdf viewer.
  The nice thing about reading papers on your screen is that you can
  zoom to the original image resolution.  This will also be the case
  for the pdf file of your contribution obtained via ADS.  Note that
  the Steinfest editors found this figure too dark and photoshopped it
  brighter for the printed book.  As author I don't really care; most
  readers will rather print a pdf on a lower-resolution printer, or
  view this image on their screen.  Readers that really want to
  appreciate the straws better zoom in on the pdf.  Note that the
  caption is set in small font so putting text in captions rather than
  the main text saves space.
% 
}\end{figure}
%===========================================================================


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\section{Evidence}                   \label{rutten-sec:evidence}
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Figure~\ref{rutten-fig:limb} shows \CaIIH\ ``straws'' at right: long
thin emission features in \CaIIH, in rows jutting out from active
network, seen near the limb against a dark background of reversed
granulation.  The latter is photospheric and is sampled only slightly
deeper in the other two images.

The VAULT-2 \Lyalpha\ images at
\url{http://wwwsolar.nrl.navy.mil/rockets/vault/archives.html}
%
  (\cf\ \cite{2001SoPh..200...63K}) % Korendyke++ VAULT1
%
show dense, 5000\,km-high hedge rows of abruptly ending bright upright
straws above network near the limb.  Comparison of the \CaIIH,
\Halpha, and \Lyalpha\ scenes show:

\leftmargini=3ex
\begin{itemize} \itemsep=0ex \vspace*{-1ex}

  \item Similarities: how can these various structures appear
        simultaneously in \Lyalpha, \Halpha, and \CaIIH?  

  \item Differences: the hedge rows of upright straws are bright and
        optically thick in \Lyalpha, bright and thin in \CaIIH, much
        less distinct and dark in \Halpha\ line center, more prominent
        but less upright and very dark in the \Halpha\ wings.  Why? 

\end{itemize}


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\section{Considerations}  \label{rutten-sec: considerations}
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The internetwork upper photosphere requires time-dependent
NLTE modeling as in the acoustic shock simulation of
%
  \citet{1997ApJ...481..500C}, %C Carlsson+Stein, K2v grain simulation
%
but does not produce noticeable \CaIIH\ emission outside acoustic
grains because the shocks do not heat on average.
See also 
%
  \citet{2005ASPC..336...25A}. %% Asplund++, test for Gene Avrett
%



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\acknowledgements We thank the conference organisers for a very good
meeting and Rob Rutten for an excellent template.


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%% References
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%RR I used the following two commands to generate the bibliography
%RR automatically with BibTeX, and then inserted the resulting .bbl file

%%\bibliographystyle{rjr-asp-bib}      %RR my file rjr-asp-bib.bst 
%%\bibliography{/tmp/adsfiles.bib}  %RR all my ADS .bib files concatenated

%RR Bibtex style rjr-asp-bib.bst doesn't treat inproceedings items
%RR the way ASP seems to like.  They should supply a better one.

%RR If the ASP doesn't get together its act re bibtex, your editor
%RR may desire you to add unique labels (such as rutten- for me) to
%RR all bibtex labels, both in the \cite commands above and after the ]{
%RR symbol combinations below.  Otherwise identical labels from another
%RR author with a worse \bibitem then yours may muck up your good work.


%RR inserted file rjr-asp-example.bbl (no change whatsoever)
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\begin{thebibliography}{}

\bibitem[\protect\astroncite{{Asplund} et~al.}{2005}]{2005ASPC..336...25A}
{Asplund} M., {Grevesse} N., {Sauval} A.~J., 2005,
\newblock in T.~G. {Barnes} III, F.~N. {Bash} (eds.), ASP Conf. Ser. 336:
  Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, \ 25

\bibitem[\protect\astroncite{{Carlsson} \& {Stein}}{1997}]{1997ApJ...481..500C}
{Carlsson} M., {Stein} R.~F., 1997,
  \apj\   481, 500

\bibitem[\protect\astroncite{{Korendyke} et~al.}{2001}]{2001SoPh..200...63K}
{Korendyke} C.~M., {Vourlidas} A., {Cook} J.~W., {Dere} K.~P., {Howard} R.~A.,
  {Morrill} J.~S., {Moses} J.~D., {Moulton} N.~E., {Socker} D.~G., 2001,
  \solphys\   200, 63

\bibitem[\protect\astroncite{{Rutten} et~al.}{2004}]{2004A&A...413.1183R}
{Rutten} R.~J., {Hammerschlag} R.~H., {Bettonvil} F.~C.~M., {S{\"u}tterlin} P.,
  {de Wijn} A.~G., 2004,
  \aap\   413, 1183

\end{thebibliography}

\end{document}

