A Prototype of a Large Tunable Fabry-Perot Interferometer for Solar Spectroscopy

Large Fabry-Perot Interferometers (FPIs) are used in a variety of astronomical instrumentation, including spectro-polarimeters for 4 m class solar telescopes. In this work we comprehensively characterize the cavity of a prototype 150 mm FPI, sporting a novel, fully symmetric design. Of particular interest, we define a new method to properly assess the gravity effects on the interferometer's cavity when the system is used in either the vertical or horizontal configuration, both typical of solar observations. We show that the symmetric design very effectively limits the combined effects of pre-load and gravity forces to only a few nm over a 120 mm diameter illuminated surface, with gravity contributing similar to 2 nm peak-to-valley (similar to 0.3 nm rms) in either configuration. We confirm a variation of the tilt between the plates of the interferometer during the spectral scan, which can be mitigated with appropriate corrections to the spacing commands. Finally, we show that the dynamical response of the new system fully satisfies typical operational scenarios. We conclude that large, fully symmetric FPIs can be safely used within solar instrumentation in both, horizontal and vertical position, with the latter better suited to limiting the overall volume occupied by such an instrument.

Automated summary

This study comprehensively characterizes the cavity of a 150 mm FPI with a novel symmetric design, showing that the design effectively limits the combined effects of pre-load and gravity forces. It also identifies a tilt variation between the plates of the interferometer during spectral scan, which can be corrected. The study demonstrates the satisfactory dynamical response of the new system to typical operational scenarios. It concludes that large, fully symmetric FPIs can be safely used in solar observations.