In-flight validation of the formation flying technologies using the ASPIICS/PROBA-3 giant coronagraph
2008
Classical externally-occulted coronagraphs are presently limited in their performances by the distance between
the external occulter and the front objective. Formation flyers open new perspectives and allow conceiving giant,
externally-occulted coronagraphs using two-spacecraft system. The PROBA-3 formation flying demonstration
mission, currently in its preparatory study phase, is intended to incorporate the ASPIICS (Association de
Satellites Pour l'Imagerie et l'Interfromtrie de la Couronne Solaire) scientific payload. ASPIICS is a solar
coronagraph designed to observe from the coronal base out to 3 solar radii with high spatial resolution in the
visible range. Formation flying technique imposes new constraints and major challenges in particular in terms
of metrology. ASPIICS will both use and demonstrate the formation flying features and performances. In order
to fully validate the formation flying technique and to improve the scientific return, original developments linked
to the formation flying constraints have been made these last years and are presented in this article.
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