Abstract
Optical bers may be used to rearrange a two-dimensional
eld of view into a slit-like conguration feeding a spectrometer. In the-
ory, such input reconguring permits two-dimensional Stokes spectrom-
etry with phase-diverse/speckle restoration to the diraction limit and
represents an alternative to adaptive optics for small telescopes. In prac-
tice, the question is whether current
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