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You are here: Technology»  HXI»  Electroformed Nickel Replication Mirror» 

Electroformed Nickel Replication Mirror

for a Hard X-ray Imager

Mirror shell configuration for X-ray optics

For soft X-rays (~1 keV), the critical angle (the angle below which x-rays can be efficiently scattered from smooth surfaces) is a few degrees, but it scales approximately inversely with energy. And this is a challenge for hard X-ray optics, because as the graze angle decreases the projected area of a mirror shell becomes very small. To overcome this one must utilize a large number of mirror shells and a focal length as long as possible. A typical mirror shell configuration first proposed by Wolter, utilizes two reflections – the first from a parabolic surface and the second from a hyperbolic surface – to produce an image that is essentially coma free. See figure below.

In addition to the primary and secondary mirror sets, the Flight Mirror Assembly (FMA) will be equipped with a straylight baffle made from aluminum to block the stray X-rays, which reached the mirror focus after only a single reflection. The size of the baffle is dependent on the cone angle of the mirror shells.

A Wolter-1 mirror configuration containing 4 nested shells

Electroformed nickel replication optic

Replicated nickel optics has been used extensively in X-ray astronomy in such missions as XMM-Newton, JETX/Swift and SAX. In the electroformed nickel replication (ENR) fabrication process, nickel mirror shells are electroformed onto a figured and superpolished aluminum mandrel. Later mirror shells are released from the mandrel using differential thermal contraction. This process was pioneered in Italy for x-ray mirror fabrication and has been used for soft-X-ray astronomy in such missions as XMM-Newton, which featured 3 mirror modules each with 68 electroformed nickel shells.

A distinct advantages of ENR are that the resulting mirror shells are inherently very stable and this stability, in turn, permits good figure accuracy, and hence very good angular resolution. Also, multiple identical copies can be made from a single mandrel and this allows the easy fabrication of multiple mirror modules. However, the high density of nickel necessitates very thin shells for the lightweight optics necessary to keep payload budget reasonable. The shells, however, proved to be strong enough to withstand the stresses of fabrication and subsequent handling without being permanently deformed.

Pictures are credit of Brian D. Ramsey and Martin C. Weisskopf, NASA/MSFC

The Ni/Co alloy electroforming bath with the multipart platter. Click the image for a larger view

A selection of resulting mirror shells. Click the image for a larger view

A test module with 4 shells mounted. Click the image for a larger view

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Selected References

  • Design and development of the SIMBOL-X hard x-ray optics, Pareschi, G.; Attinâ, P.; Basso, S.; Borghi, G.; Burkert, W.; Buzzi, R.; Citterio, O.; Civitani, M.; Conconi, P.; Cotroneo, V. et al., SPIE vol. 7011 (2008)
  • Development of a prototype nickel optic for the Constellation-X hard x-ray telescope, Romaine, S.; Basso, S.; Bruni, R. J.; Burkert, W.; Citterio, O.; Cotroneo, V.; Engelhaupt, D.; Freyberg, M. J.; Gorenstein, P.; Gubarev, M. et al., SPIE Vol 6688 (2007)
  • Development of a prototype nickel optic for the Constellation-X hard x-ray telescope: IV, Romaine, S.; Basso, S.; Bruni, R. J.; Burkert, W.; Citterio, O.; Conti, G.; Engelhaupt, D.; Freyberg, M. J.; Ghigo, M.; Gorenstein, P.; and 8 coauthors, SPIE Vol 6266 (2006)
  • The Con-X Hard X-Ray Telescope and its angular resolution, Gorenstein, P.; Romaine, S.; HXT Integral Optics Team, AAS Vol.207 (2005)
  • Development of Prototype Nickel Optic for the Constellation-X Hard X-Ray Telescope, Romaine, S.; Gorenstein, P.; Bruni, R.; Pareschi, G.; Citterio, O.; Ghigo, M.; Mazzoleni, F.; Spiga, D.; Basso, S.; Conti, G.; and 8 coauthors, AAS Vol 207 (2005)
  • Long-term Stability and High Energy Reflectivity Measurements of Depth Graded Multilayer Coatings for X-ray Optics, Unks, B. E.; Bruni, R. J.; Eguchi, H.; Gorenstein, P.; Romaine, S. E., AAS Vol 205 (2004)

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