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Detectors
 

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Detectors

  

In order to take full advantage of the telescope resolution, both the pair of MCPs in the detector and the resistive anode readout system are curved, like a watchglass, to match the optimum focal surface. A CsI photocathode is deposited directly onto the front face of the front MCP to enhance the EUV quantum efficiency.   The detector spatial resolution is substantially (a factor >2) better than that of the mirror nest and consequently does not contribute significantly to the net performance of the WFC. A focal plane turntable can be used to select one of two identical detector assemblies in flight. Table 6.2 gives details of the detectors.

 

 

Diameter tex2html_wrap_inline14181
Active diameter tex2html_wrap_inline14183
Radius of curvature tex2html_wrap_inline14185
Channel diameter tex2html_wrap_inline14187
Channel pitch tex2html_wrap_inline14189
Open area 63%
Length-to-diameter ratio 120:1
Front MCP bias angle tex2html_wrap_inline14191
Rear MCP bias angle tex2html_wrap_inline14193
Photocathode (front MCP only) tex2html_wrap_inline14195 CsI
Table 6.2: WFC detector characteristics



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