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The importance of scientific visualization has often been
discussed in this space in the past, and with good reason.
Experiments and simulations produce reams of data that
must be analyzed and understood by the scientists producing them,
which can be a daunting task. And even though researchers
involved in a project may develop the ability to visually scan
numbers and glean some meaning, communicating their significance
to others is often nearly impossible without some sort of
graphical representation. Many products and protocols have
been developed for converting numbers to pictures, but when it
comes to analyzing astronomical data, many scientists can often
be found playing with the AIPS.
Even without knowing much about the physics of the problems for which AIPS is commonly employed, a brief survey of its features is quite impressive and gives one a general feel for the quantity and quality of programming effort which has been involved, estimated at well over 60 man years. The AIPS package has evolved into the primary software package for displaying and analyzing radio images of two or three dimensions. Moreover, it serves as both an interactive tool and a batch processing program, allowing maximum flexibility for the user. In addition, there are several megabytes of documentation provided to guide the researcher in his visualization efforts. In addition to the above features, AIPS has been developed with optimum performance and portability in mind. Written primarily in Fortran and C (generally fast computational languages), AIPS was written in a general way to make porting from one computer platform to another relatively seamless and painless. As a general rule, when developing with an eye toward portability, minimal changes should be needed to the source code, with differences being more or less confined to compiler directives. AIPS appears to have done a nice job here, too, limiting source Go To Page: 1 2
The copyright of the article Analyzing Astronomical Data Can Drive You (to) AIPS!
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