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Proceedings Paper • Open Access

Final results of the PERSEE experiment
Author(s): J.-M. Le Duigou; J. Lozi; F. Cassaing; K. Houairi; B. Sorrente; J. Montri; S. Jacquinod; J.-M. Réess; L. Pham; E. Lhomé; T. Buey; F. Hénault; A. Marcotto; P. Girard; N. Mauclert; M. Barillot; V. Coudé du Foresto; M. Ollivier

Paper Abstract

The PERSEE breadboard, developed by a consortium including CNES, IAS, LESIA, OCA, ONERA and TAS since 2006, is a nulling demonstrator that couples an infrared nulling interferometer with a formation flying simulator able to introduce realistic disturbances in the set-up. The general idea is to prove that an adequate optical design can considerably release the constraints applied at the spacecrafts level of a future interferometric space mission like Darwin/TPF or one of its precursors. The breadboard is now fully operational and the measurements sequences are managed from a remote control room using automatic procedures. A set of excellent results were obtained in 2011: the measured polychromatic nulling depth with non polarized light is 8.8x10-6 stabilized at 9x10-8 in the [1.65-2.45] μm spectral band (37% bandwidth) during 100s. This result was extended to a 7h duration thanks to an automatic calibration process. The various contributors are identified and the nulling budget is now well mastered. We also proved that harmonic disturbances in the 1-100Hz up to several tens of nm rms can be very efficiently corrected by a Linear Quadratic Control (LQG) if a sufficient flux is available. These results are important contributions to the feasibility of a future space based nulling interferometer.

Paper Details

Date Published: 20 November 2017
PDF: 12 pages
Proc. SPIE 10564, International Conference on Space Optics — ICSO 2012, 105640E (20 November 2017); doi: 10.1117/12.2309220
Show Author Affiliations
J.-M. Le Duigou, Ctr. National d'Études Spatiales (France)
J. Lozi, ONERA (France)
Groupement d’Intérêt Scientifique PHASE (France)
F. Cassaing, ONERA (France)
Groupement d’Intérêt Scientifique PHASE (France)
K. Houairi, ONERA (France)
Groupement d’Intérêt Scientifique PHASE (France)
B. Sorrente, ONERA (France)
Groupement d’Intérêt Scientifique PHASE (France)
J. Montri, ONERA (France)
Groupement d’Intérêt Scientifique PHASE (France)
S. Jacquinod, Institut d'Astrophysique Spatiale d'Orsay (France)
J.-M. Réess, Observatoire de Paris (France)
Groupement d’Intérêt Scientifique PHASE (France)
L. Pham, Observatoire de Paris (France)
E. Lhomé, Observatoire de Paris (France)
Groupement d’Intérêt Scientifique PHASE (France)
T. Buey, Observatoire de Paris (France)
F. Hénault, Observatoire de la Côte d'Azur (France)
A. Marcotto, Observatoire de la Côte d'Azur (France)
P. Girard, Observatoire de la Côte d'Azur (France)
N. Mauclert, Observatoire de la Côte d'Azur (France)
M. Barillot, Thales Alenia Space (France)
V. Coudé du Foresto, Observatoire de Paris (France)
M. Ollivier, Institut d'Astrophysique Spatiale d'Orsay (France)


Published in SPIE Proceedings Vol. 10564:
International Conference on Space Optics — ICSO 2012
Bruno Cugny; Errico Armandillo; Nikos Karafolas, Editor(s)

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