\documentclass[referee]{/home/raid/astro/gd232/papers/aa-package/aa}
%\documentclass[times]{aa}

% tth -e2haicV -Ltalk < talk.tex >! all.htm


\usepackage{epsfig}
\usepackage{psfig}

\input{/home/raid/astro/gd232/papers/definitions.tex}

%\input{def_journals.tex}

\usepackage{natbib}
\bibpunct{(}{)}{;}{a}{}{,} %for A&A style

\def\hyperlink#1#2{\special{html:<a href="\##1">}#2\special{html:</a>}}
  % Incorrect link name in \TeX\ because # can't be passed properly to a special.
\def\hypertarget#1#2{\special{html:<a name="#1">}#2\special{html:</a>}}
\long\def\tthdump#1{#1} % Do nothing. The following are not done for TtH.
\tthdump{%
\def\title#1{\bgroup\leftskip 0 pt plus1fill \rightskip 0 pt plus1fill
\pretolerance=100000 \lefthyphenmin=20 \righthyphenmin=20
\noindent #1 \par\egroup}% Centers a possibly multi-line title.
 \let\author=\title % Actually smaller font than title in \LaTeX.
 \input epsf     % PD package defines \epsfbox for figure inclusion
  % Macro for http reference inclusion, per hypertex.
 \def\href#1#2{\special{html:<a href="#1">}#2\special{html:</a>}}
 \def\urlend#1{#1\endgroup}
 \def\url{\begingroup \tt 
  \catcode`\_=13 % Don't know why this works.
  \catcode`\~=11 \catcode`\#=11 \catcode`\^=11 
  \catcode`\$=11 \catcode`\&=11 \catcode`\%=11
\urlend}% \url for plain \TeX.
}

% gs -dSAFER -xResolution=50 -yResolution=50 -dNOPAUSE
% -sDEVICE=pdfwrite -sOutputFile=draft.pdf paper3.ps 


\begin{document}


\title{Multi-wavelength observations of compact solar flares }

\centerline{G. Del Zanna}

\centerline{H.E. Mason DAMTP, University of Cambridge, UK}

\centerline{A. Berlicki,  B. Schmieder (Observatoire de Paris,Meudon)}


\tableofcontents

\section{Introduction}


\bi
\item
The SOHO/Coronal Diagnostic Spectrometer provides essential  
spectroscopic information to understand the characteristics 
and dynamics of solar coronal features.

\item
We give a description of the main observational features
and what types of measurements (densities, temperatures, flows)
are obtained. 

\item
These provide important observational constraints 
for flare modeling.

\item
 CDS observations of a compact M1 flare 
that occurred on October 22 2002, also observed from the ground
in chromospheric lines  and by RHESSI.

The flare occurred in a region of strong and mixed magnetic polarity,
was compact and lasted only a short time.
\ei

\subsection{paper}

\begin{figure}[!htbp]
\centerline{\epsfig{file=p1.ps, width=9.0cm,angle=0 }}
\end{figure}

\section{Overview}

\begin{figure}[!htbp]
\centerline{\epsfig{file=fov.ps, width=9.0cm,angle=0 }}
\end{figure}

\begin{figure}[!htbp]
\centerline{\epsfig{file=wl.ps, width=9.0cm,angle=0 }}
\centerline{\epsfig{file=blong.ps, width=9.0cm,angle=0 }}
\caption{THEMIS/MSDP in  Na I ${\rm{D_{1}}}$
(15:41--16:29 UT) and line-of-sight magnetic field deduced from
           $I$ and $V$ Stokes overlaid with H$\alpha$ contours
observed by VTT/MSDP at 15:30:01 UT.}
\end{figure}

\begin{figure}[!htbp]
\centerline{\epsfig{file=goes.ps, width=9.0cm,angle=0 }}
\end{figure}

 THEMIS observed continuously between 15:41--17:26 UT.

TRACE and VTT/MSDP observations were performed during 
           the whole flare.

VTT/MSDP observations in H$\alpha$
9 scans between 15:30 and 16:17 UT


TRACE high cadence (40 s) in the 195 {\AA} band between 15:29 and
15:41 UT 



\begin{figure}[!htbp]
\centerline{\epsfig{file=rhessi_cr.ps, width=9.0cm,angle=0 }}
\caption{RHESSI counts rates (the 12--25 keV  band are 
multiplied by a factor of 10).
}
\end{figure}

\section{Pre-flare}

\subsection{Overview}

\begin{figure}[!htbp]
\centerline{\epsfig{file=trace_195_12:23_cds.ps, width=9.0cm,angle=0 }}
\centerline{\epsfig{file=trace_195_12:23_mdi.ps, width=6.0cm,angle=0}
}
\end{figure}

\subsection{CDS rasters}

\begin{figure}[!htbp]
\centerline{\epsfig{s26054r01_ima.ps, width=9.0cm,angle=0 }
\centerline{\epsfig{s26054r01_pos.ps, width=9.0cm,angle=0 }
\end{figure}

\begin{figure}[!htbp]
\centerline{\epsfig{s26055r00_ima.ps, width=9.0cm,angle=0 }
\centerline{\epsfig{s26055r00_pos.ps, width=9.0cm,angle=0 }
\end{figure}

\subsection{Small Flare - C class}

\begin{figure}[!htbp]
\centerline{\epsfig{s26056r00_ima.ps, width=9.0cm,angle=0 }
\end{figure}



\section{Movies!}

{\bf MDI}
\url{movie_mdi_long.html} ~~(\url{movie_mdi_long.mpg})

{\bf MDI - during the M1 flare}
\url{movie_mdi_15_16.html} ~~(\url{movie_mdi_15_16.mpg})

{\bf TRACE 195 \AA}
\url{movie_trace.html} ~~(\url{movie_trace.mpg})


\section{The M1 flare}


\begin{figure}[!htbp]
\centerline{\epsfig{file=trace_195_154039_mdi.ps, width=9.0cm,angle=0 }}
\centerline{\epsfig{file=trace_195_154039_FeXIX_int.ps, width=9.0cm,angle=0 }}
\caption{Top: TRACE 195 \AA\ + MDI contours
Bottom: CDS FOV - TRACE 195 \AA\ + contours of Fe XIX intensity
}
\end{figure}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=s26058r00_HeI_int_mdi.ps, width=6.0cm,angle=0 }
\epsfig{file=s26058r00_HeI_pos_mdi.ps, width=6.0cm,angle=0}
}
\end{figure}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=s26058r00_OV_int_mdi.ps, width=6.0cm,angle=0 }
\epsfig{file=s26058r00_OV_pos_mdi.ps, width=6.0cm,angle=0}
}
\end{figure}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=s26058r00_SiXII_int_mdi.ps, width=6.0cm,angle=0 }
\epsfig{file=s26058r00_SiXII_pos_mdi.ps, width=6.0cm,angle=0}
}
\end{figure}

\subsection{Zoom in}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=s26058r00_FeXIX_int_mdi.ps, width=6.0cm,angle=0 }
\epsfig{file=s26058r00_FeXIX_int_SiXII_pos.ps, width=6.0cm,angle=0}
}
\end{figure}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=s26058r00_FeXIX_pos_SiXII_pos.ps, width=6.0cm,angle=0}
\epsfig{file=trace_195_154039_SiXII_pos.ps, width=6.0cm,angle=0}
}
\end{figure}


\section{Post-flare CDS raster 15:43--17:07 UT}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=s26059r00_ima.ps, width=6.0cm,angle=0}
}
\end{figure}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=s26059r00_pos.ps, width=6.0cm,angle=0}
}
\end{figure}

\begin{figure}[!htbp]
\centerline{
\epsfig{file=trace_1627_FeXIX_int.ps, width=6.0cm,angle=0}
}
\end{figure}


\begin{figure}[!htbp]
\centerline{
\epsfig{file=rhessi_1625_1628_3kev.ps, width=6.0cm,angle=0}
}
\end{figure}


%\begin{figure}[!htbp]
%\centerline{\epsfig{file=pp.eps, width=9.0cm,angle=0 }}
%\caption{MDI contour levels on SXT image=100,200,500 G}
%\end{figure}



\section{Conclusions}

\bi
\item
Strong blue-shifts in lines emitted in the 1-8 MK range are observed
at the bases of hot Fe XIX structures.

\item
The hot structures are also clearly visible in the TRACE 195~\AA\ band

\item
The hot structures match the thermal emission as seen by RHESSI

\ei

\noindent
{\bf Acknowledgements}

Support from  PPARC is acknowledged.



\bibliographystyle{aa}
%\bibliography{/home/raid/astro/gd232/papers/bib}
%\bibliography{talk}

\end{document}
