After you take Foucault Test Measurements, you need to process, or reduce, the data, to understand the shape of your mirror surface. When this is determined, you can decided which zones to work on, or declare the mirror done.
Before computers were common, the data reduction was done manually. Many of the mirror making books listed in our bibliography will describe the steps to do this. [Texerau84] has the most through description, a nice worksheet to use, and is by far the most popular.
| Program | Platform | Author(s) | Web Site | Comments |
| Figure | DOS* | Dave Rowe |
http://members.aol.com/aplanatic/figure45.htm | Good Interface and Nice Plots |
| Figure XP | Windows XP | Dave Rowe James Lerch |
http://lerch.no-ip.com/atm/FigureXP.zip
(Exe only 140KB) http://lerch.no-ip.com/atm/FigureXP_Full.zip (Full install 1.47MB) |
Newer version of above with Star Test Simulator |
| Tex | DOS*, Mac, Linux X86, Solaris, HP-UX |
Mike Lindner |
http://home.att.net/~mikel/index.html | Faithful to Texerau's "Test Sheet" |
| Six Tests | DOS* Windows |
Jim Burrows |
http://home.earthlink.net/~burrjaw/atm/ | Foucault, Caustic Poorman's both Fixed and Moving Source. |
| Couder | Windows | Ricardo Dunna |
http://www.atmsite.org/contrib/Dunna/foucault/index.html | Can track figuring progress |
| Foucault Test Image Analyzer |
Any Java Platform |
Dejan Vucinic | http://foucault.sourceforge.net/ | Multi-platform |
| *DOS program run under Windows in DOS mode. | ||||
Page last edited 2007-Sep-23