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Published on: August 4, 2018
External occulter laboratory demonstrator for the forthcoming formation flying coronagraphs.
Federico Landini1, Sébastien Vives, Mélanie Venet
1Dipartimento di Fisica e Astronomia, Università di Firenze, Firenze, Italy. flandini@arcetri.astro.it
Researchers tested a new coronagraph demonstrator for formation flight missions. This research confirms findings on smaller coronagraphs and offers insights into optimizing occulter geometry for future solar observation spacecraft.
Area of Science:
- Space optics and instrumentation
- Solar physics
- Astrophysics
Background:
- External occulter geometry is critical for solar coronagraph performance.
- Formation flight coronagraphs offer improved capabilities but pose mechanical and alignment challenges.
- Minimizing diffraction from occulter edges is essential for sensitive solar observations.
Purpose of the Study:
- To design and test a demonstrator for a formation flight solar coronagraph.
- To investigate the optimization of external occulter geometry for enhanced solar imaging.
- To validate laboratory test results with existing research on smaller coronagraphs.
Main Methods:
- Design of a linear edge coronagraph demonstrator.
- Laboratory testing of the demonstrator's optical performance.
- Analysis of occulter geometry and tolerance optimization.
Main Results:
- Confirmed findings from previous studies on smaller coronagraphs.
- Provided data on the geometry and tolerances for occulter optimization.
- Demonstrated the feasibility of testing coronagraph components in a laboratory setting.
Conclusions:
- The study validates the optimization approach for coronagraph occulter geometry.
- Results contribute to the development of next-generation formation flying solar coronagraphs.
- Further research may be needed to extrapolate findings to circular occulters.
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