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eso-midas-doc-13SEPpl1.2-3.mga5.i586.rpm

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<H1><A NAME="SECTION00420000000000000000">&#160;</A> 
<A NAME="general-concept-of-midas">&#160;</A>
<BR>
General Concept of MIDAS
</H1> 
The MIDAS system is built along lines which should allow easy
integration of complex analysis algorithms as well as allowing greater
flexibility in interactive use and in the creation of user specific
procedures from the basic building blocks. The first design proposal
for MIDAS, made late 1980, used some ideas from the UK STARLINK
project for the software interface definitions.  The present version
which became available in 1984 follows a similar philosophy in its
application program interfaces, but has been expanded to the new
Standard Interfaces which have a broader base than previously.

<P>
MIDAS has benefitted greatly from the experience gained at ESO using
the Hewlett-Packard based image processing system IHAP (see F.
Middelburg, IHAP Manual, ESO 1985). Not only have many of the internal
design features such as ``world coordinates'' been incorporated, but
also the command language has been designed in such a way that it is
similar to the basic philosophy of IHAP.

<P>
The MIDAS system can be run in both an interactive and a batch mode.
In addition, the interactive user will be able to create batch jobs
which will run in parallel with the interactive work.

<P>
MIDAS is based on three sets of general interfaces for application
programs to data structures, namely: a) the ``Standard Interfaces''
for general I/O and image access, b) the ``Table Interfaces'' for
access to table structures, and the ``Graphics Interfaces'' for 
data representation in graphical format. These interfaces allow easy 
integration of application programs into MIDAS.  To provide a portable 
system a layer of OS-routines have been used to shield MIDAS from 
the local operating system. These routines may only be used at lowest 
levels and are not available for normal applications.

<P>
To facilitate easy implementation of different graphic and display
devices, MIDAS has adopted a set of device independent interfaces for
plotting and image display. All plotting routines in MIDAS are based
on the <B>A</B>STRONET <B>G</B>raphic <B>L</B>ibrary, developed and
maintained by the italian ASTRONET. Further, the image display
applications are using the <B>I</B>mage <B>D</B>isplay <B>I</B>nterface
routines defined in collaboration with ST&nbsp;ScI, UK STARLINK, KPNO and
Trieste Observatory.

<P>
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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-09</I>
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