VForiel / Tunable-Kernel-Nulling

(PhD) Adaptive tunable kernel-nulling interferometry for the direct detection of extrasolar planets
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Reduction of degrees of freedom #44

Closed VForiel closed 1 week ago

VForiel commented 5 months ago

Discussed in https://github.com/Leirof/Tunable-Kernel-Nulling/discussions/31

Originally posted by **Leirof** March 4, 2024 Some degree of freedom seems redoundant, such as $P_1$ which can be removed and use the first input's phase as the reference phase. We can also consider removing $P_9$, $P_{10}$ and $P_{12}$ for the same reason. Does it work as expected? Can we also consider removing $P_3$, $P_5$ and $P_6$? ![dof_reduction](https://github.com/Leirof/Tunable-Kernel-Nulling/assets/12165342/9e60fbb3-20f4-4927-89fe-382042da467c)
VForiel commented 2 weeks ago

By adding the phase plots to the manual shift control interface and playing with it, I noticed that, for any initial perturbations, there is a way of optimizing the system using only P2, P3, P4, P6, P9, P10 and P12

Random initial state: image

By playing with P2, P3 and P4 only, it is possible to optimize the bright output (and the first null output at the same time) image

I can then correct the phases for the null output 2 and 3 by playing only with P6 (or alternatively with P7) image

Finally, I can do the same for each pair of dark output by modifying only one of the two shifters before each cross recombiner image

Unfortunately, this process require to know the phases at different points in the system, which is an information we don't have access to in practice. Thus, there is no straightforward implementation of this method.

Additionaly the current calibration algorithme seems very affected by the reduction of the degree of freedoms as it has more trouble to converge to a satisfying solution, and this solution seems often less good than when I let the algorithme play with all the degree of freedom.

image image