Current progress on TPF-I mid-infrared achromatic nulling at the Jet Propulsion Laboratory
2007
Infrared interferometric nulling is a promising technology for exoplanet detection. Nulling
research for the Terrestrial Planet Finder Interferometer has explored several interferometer architectures at
the Jet Propulsion Laboratory (JPL). The most recent efforts have focused on an architecture which
employs a geometric field flip to achieve the necessary π phase delay in the interferometer. The periscope
design currently in use allows for a completely achromatic phase flip. Deep interferometric nulling
requires optical path stability, precision optical alignment, intensity balancing, and dispersion correction.
This paper will discuss recent efforts to implement a precision optical alignment, stabilize the
interferometer environment, implement optical path metrology, control intensity balance, and compensate
for dispersion introduced by beamsplitter mismatch.
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