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\documentstyle[psfig,12pt]{joso}
\begin{document}

\def\proca{?? (ed.): {\sf JOSO Annual Report '99}}
\def\procb{\copyright 1999 Astronomical Institute, Tatransk\' a Lomnica --
   Printed in Slovakia}
  %RE above lines are for you


%%\def\figs{/f4-usr1/rutten/art/DOT/1996}
%%\def\figs{.}

\title{SOLAR PHYSICS IN THE NETHERLANDS --- 1998\\[1ex]}
  %RR they want capitals; extra space needed

\author{Rob RUTTEN\inst{1}, 
        Rony KEPPENS\inst{2} 
          \and 
        Bernhard FLECK\inst{3}\\[2ex]}
  %RR they want family names capitals - strange French habit?

\institute{Sterrekundig Instituut Utrecht,
           Postbus 80\,000, NL-3508~TA Utrecht, 
           The Netherlands\\[-1ex]
        \and
           FOM Institute for Plasma Physics Rijnhuizen,
           Postbus1207, NL--3430~BE Nieuwegein,
           The Netherlands\\[-1ex]
        \and
           ESA Space Science Department,
           Postbus 299, NL--2200~AG Noordwijk,
           The Netherlands\\[2ex]
        }
    %RR they want full postal addresses; add spacings as above

\maketitle
        
\parindent=0ex \parskip=2ex \large

Solar physics research in the Netherlands is carried
out at Utrecht, Nieuwegein and Noordwijk.

At the {\em Sterrekundig Instituut Utrecht} solar physics was 
done by Rob Rutten with graduate students 

Rob Hammerschlag's Dutch Open Telescope (DOT) came to a standstill

Another 1998 activity was the start of the
EU-TMR-funded European Solar Magnetometry Network


At the {\em Utrecht Space Research Institute}, a non-University
institute, partial interests in solar physics are retained by Peter
Hoyng (dynamo theory), Rolf Mewe and Jelle Kaastra (plasma
diagnostics).


%%%% Rony - your job to update the below
At the {\em FOM Institute for Plasmaphysics\/} at Nieuwegein (also
non-University) Hans Goedbloed leads a plasma
physics group that in 1998 included Rony Keppens (postdoc) and
graduate students Bart van der Holst and Ronald Nijboer.  Ronald
succesfully defended his thesis ``Waves and Instabilities of
Magnetohydrodynamic Flows in Flux Tubes'' in 1998.  The group
concentrates on linear and nonlinear MHD aspects of laboratory and
astrophysical plasmas using analytical and numerical methods.  
%% Topics include stationary MHD flow solutions (e.g. modeling solar and
%% stellar transonic outflows), spectral MHD characteristics of
%% tokamaks and stratified plasmas with background flow, and large-scale
%% numerical simulations. 
     %% too long, Rob
Examples are shown at
{\tt http:/$\!$/www.phys.uu.nl/}$\sim${\tt mpr/} and
{\tt http:/$\!$/www.phys.uu.nl/}$\sim${\tt toth/}.

%%%%% Bernhard - your job to update the below
At {\em ESTEC\/} (Noordwijk) there is an international
(and rather transient) ESA solar physics group
that is involved, among other projects, in SOHO and Ulysses. 
At the end of 1998 the group at ESTEC consisted of 
Martin Huber (Head ESA Space Science Department),
Peter Wenzel (Head of the Solar System Division; Ulysses data),
Vicente Domingo (irradiance variations, SOHO data, SOHO Project Scientist
until 30 June 1998)
Bernard Foing (solar and stellar spectroscopy),
Thierry Appourchaux (helioseismology, SOHO),
William Chaplin (research fellow, helioseismology, SOHO and BISON data,
from October 1998)
Richard Marsden (Ulysses),
Trevor Sanderson (Ulysses),
David Lario (research fellow, energetic particles, Ulysses data),
Karin Muglach (research fellow; chromospheric fields and 
dynamics, SOHO/GCT+VTT data; until October 1998),
Salvatore Orlando (research fellow; Coronal Loops, SOHO/Yohkoh data),
Milan Maksimovic (research fellow; Solar Wind, Ulysses data)
and
David Lario (research Fellow; ion acceleration, Ulysses data)

Finally, the {\em SOHO Project Scientist Team\/} consisting of
Bernhard Fleck (SOHO Deputy Project Scientist since 1 July 1998; 
                  chromospheric oscillations),
Luis Sanchez (SOHO Science Data Coordinator; helioseismology),
Piet Martens (SOHO Science Operations Coordinator; coronal heating 
and flares),
Alexander Belien (ESA external research fellow;
   coronal heating, MHD modelling),
and
Jack Ireland (ESA external research fellow; coronal heating, MHD modelling)
resided at Goddard Space Flight Center in Greenbelt, Maryland.

\end{document}




%========================================================= fig_xx
\begin{figure}[htbp]  %% max 134mm
  \centerline{\psfig{figure=\figs/dot_rdlm_skyline_small.eps,%
           bbllx=125bp,bblly=395bp,bburx=500bp,bbury=550bp,clip=t,%
                     width=\textwidth}}
  \vspace*{5mm}
  \centerline{\psfig{figure=\figs/dot_open_svst_small.eps,%
           bbllx=100bp,bblly=340bp,bburx=500bp,bbury=550bp,clip=t,%
                     width=\textwidth}}
    \caption[]{\label{fig_skyline}
     First images from the DOT, November 1997.
     bla bla 
     }  
\end{figure} 
%================================================================