TPF-C Technology Plan - Exoplanet Exploration Program - NASA
TPF-C Technology Plan - Exoplanet Exploration Program - NASA
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 />
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