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TPF-C Technology Plan - Exoplanet Exploration Program - NASA

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Optics and Starlight Suppression <strong>Technology</strong><br />

3.1.5 Transmissive Optics<br />

Objective<br />

The minimum mission design incorporated two features that make use of large (greater than<br />

10-cm clear aperture) transmissive optics. The first is a polarizer assembly consisting of a<br />

polarizing beam splitter (PBS) and two additional cubes required to achieve the required<br />

extinction while compensating for the chromatic dispersion. The polarizer assembly serves to<br />

give two separate paths for two orthogonal polarizations, each with its own set of deformable<br />

mirrors and downstream optics. The second feature is a Michelson assembly, chosen over the<br />

Mach-Zehnder due to its compactness, which accommodates wavefront control via the two DMs<br />

in each path. The total path in the glass for each sub-system is on the order of 25 cm.<br />

The objective of this effort is to identify and, if necessary, address materials issues involved in<br />

the fabrication of large transmissive optics to the required tolerances, such as the uniformity of<br />

the glass, stress birefringence, scatter and depolarization, and the chromatic variation of these.<br />

Approach<br />

The preferred approach to addressing this technology risk is to develop design options that<br />

bypass entirely or reduce the dependence on transmissive optics. Several trades are still open in<br />

the coronagraph design and may result in the elimination of the two separate polarization paths<br />

or modification of the interferometric configuration. There are two main options. The first one<br />

is to control polarization through special coatings on the mirrors along with design changes that<br />

will allow elimination of the second polarization beam path. The second one is the introduction<br />

of a non-interferometric DM arrangement, thus removing another large transmissive optic.<br />

Polarization control through mirror coating is an ongoing effort. Concepts for polarizationinsensitive<br />

occulting masks are also being considered.<br />

However, if it is decided that a configuration similar to that of the minimum design mission is<br />

needed, the technology development will be planned and initiated in Phase A.<br />

Progress to Date<br />

Progress to date has consisted solely of initial investigation into the state-of-the-art; detailed<br />

requirements have not yet been developed for transmissive optical elements.<br />

Homogeneity<br />

Published data for fused silica 15 show homogeneity values in the range of 0.5 ppm. These were<br />

assessed with blanks ~200 mm in diameter and ~50 mm thick. Wavefront error of less than<br />

~0.007 waves rms is achievable with blank selection. Homogeneity is determined from the p-v<br />

net wavefront error upon transmission for any given blank. It therefore leaves unanswered the<br />

question of spatial distribution, which would need further study. For other optical glasses, the<br />

Schott glass catalog shows values of 1 ppm as achievable depending on the type of glass and<br />

15 J. L. Ladison et al., “Achieving low wavefront specifications for DUV lithography; impact of residual<br />

stress in HPFS® fused silica,” Proc. SPIE 4346, 1416-1423 (2001).<br />

41

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