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Description

(pre-alpha)
Main purpose of this project is to reconstruct telescope's mirror shape by pre- and postfocal Hartmann images (classical Hartmann test).
In future there's plans to work also with Shack-Hartmann.

Secondary abilities of this project:
- FITS-viewer with some simple functionality;
- 3D image viever;
- simple operations with FITS images.

fitsview-hartmann Web Site

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Additional Project Details

Languages

Russian

Intended Audience

Science/Research

User Interface

GTK+

Programming Language

C

Registered

2012-07-20
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