On 2007-06-01 15:18-0700 Jerry wrote:

> [...]To summarize: The plan is to make a quasi-third Ada binding which is
> exactly like the current thick binding except that the subroutine
> names are the traditional PLplot names. There will be two example
> files for each example, one written to the thick binding and one
> written to the new binding. The naming conventions are e.g. for
> Example 1, xt01a.adb is written for the thick binding and x01a.adb is
> written to the new binding.
>
> Coding for the Ada examples should use Ada constructs and functions
> as needed. (See the other note from me today relating to the sprintf
> problem from a few days ago.)
>
> Once an example is complete for one binding, the corresponding
> example can be automatically generated by a series of string
> substitutions for subroutine names on the source--that's how I plan
> to generate the new binding as well.

Sounds like an excellent plan.

Alan
__________________________
Alan W. Irwin

Astronomical research affiliation with Department of Physics and Astronomy,
University of Victoria (astrowww.phys.uvic.ca).

Programming affiliations with the FreeEOS equation-of-state implementation
for stellar interiors (freeeos.sf.net); PLplot scientific plotting software
package (plplot.org); the libLASi project (unifont.org/lasi); the Loads of
Linux Links project (loll.sf.net); and the Linux Brochure Project
(lbproject.sf.net).
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