The third stage in the evolution of my solar equipment replaced the refracting telescope described here with a Newtonian reflector. The goal of this change was to achieve greater resolution than was possible with a 4.5 inch aperture system. Since I wanted to approximately double the resolution I needed to double the aperature. This was not feasible with a refractor because of cost. A refractor also requires either front aperture filtration or dealing with a very hot prime focus image. Larger aperture is relatively inexpensive in a reflector and the use of an uncoated primary mirror provides enough decrease in the concentrated light to make it managable. I chose an open truss tube structure to minimize the build-up of thermal gradients in the air surrounding the mirrors.

The primary mirror is an 8", f/10 (80" focal length), 1/20l, unaluminized, full thickness, Pyrex paraboloid. The mirror cell is painted white to minimize its heat-up while observing and, hence, stresses that would deform the figure of the mirror. Others have used black mirror mounts on the thinking that reflected light from the mount would reduce the contrast in the image by an intolerable amount. I have not found that to be true. The path back to the camera detector requires many reflections off of surfaces that are painted black. There is also a field stop that restricts the entrance angle of any scattered light an a narrow band optical filter that restricts the wavelength of light that can reach the detector.
Uncoated Pyrex has a reflectivity of about 5% and the reflectivity of the coated secondary is probably not much better than 85% since it is several years old. Consequently, the flux at prime focus is only about 5 times greater than normal incidence sun light. This flux is still more than adequate to do permanent and instant damage to ones eyes! This telescope design is not intended for visual use and such a telescope should never be used visually. No where on this telescope is there an eyepiece. The entire instrument package is electronic (video) as described here.

Page Last Updated: 27 June 2001

Copyright © 2001 Arthur L. Whipple, All Rights Reserved