Co-phasing a segmented mirror telescope using a deformable mirror and phase diversity
For small satellite remote sensing missions, a large aperture telescope which has more than 400 mm of diameter is required to realize less than 1m GSD observations. However, it is difficult or expensive to realize the large aperture telescope using monolithic primary mirror with high surface accurac...
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Main Author | |
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Format | Conference Proceeding |
Language | English |
Published |
SPIE
06.09.2019
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Online Access | Get full text |
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