I've recently created a software that can help to evaluate the thermal
behavior of a telescope mirror. Here's a screen shot of the application:
www.cruxis.com/scope/img/MirrorCooling_1.gif .
The application simulates the temperature evolution in a mirror subject
to varying ambient temperature and chosen heat transfer conditions on
the front and back surface. It displays a plot of the temperature
profile at every time step, and a graph of the evolution of the mirror
core, optical surface and air temperature.
You can download the software:
www.cruxis.com/scope/download/MirrorCooling.zip . The archive contains a
single executable file MirrorCooling.exe.
The following parameters are used by the program:
- Mirror Thickness
- Initial Mirror Temperature
- Initial and Final Air Temperature (varying linearly between start and
end)
- Film Coefficients for front and back (recommended values are between 5
and 15 without fans, between 20 and 100 with fans)
- Radiation Coefficients for front and back (0.04 for aluminum coating
on front surface)
- Simulation duration and time step
It's amazing to see how slowly a 2" thick mirror cools if no fans are
installed. And with thinner mirrors you can see how the temperature
drops below the ambient air temperature because of the heat radiation to
the sky.
Any comments, questions or suggestions about the software are welcome.
Cheers,
Robert Houdart
www.cruxis.com/scope