SP-436 Project Orion: A Design Study of a System for Detecting Extrasolar Planets

Figure 7. A plat of the root-mean-square optical path difference <(L22>1/2) as a function of interferometer baseline (B). Solid curves pertain to differing assumptions concerning the turbulence outer scale (L0); crosses refer to data discussed in appendix A.

Figure 7. A plat of the root-mean-square optical path difference <(L22>1/2) as a function of interferometer baseline (B). Solid curves pertain to differing assumptions concerning the turbulence outer scale (L0); crosses refer to data discussed in appendix A.

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