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dc.contributor.authorCahoy, Kerri
dc.contributor.authorCheng, Kezi
dc.contributor.authorJamil, Sara
dc.contributor.authorMarinan, Anne D.
dc.contributor.authorKerr, Caitlin E.
dc.date.accessioned2013-09-23T12:34:11Z
dc.date.available2013-09-23T12:34:11Z
dc.date.issued2012-08
dc.date.submitted2012-07
dc.identifier.issn0277-786X
dc.identifier.urihttp://hdl.handle.net/1721.1/80847
dc.description.abstractThe goal of the CubeSat Deformable Mirror Demonstration (DeMi) is to characterize the performance of a small deformable mirror over a year in low-Earth orbit. Small form factor deformable mirrors are a key technology needed to correct optical system aberrations in high contrast, high dynamic range space telescope applications such as space-based coronagraphic direct imaging of exoplanets. They can also improve distortions and reduce bit error rates for space-based laser communication systems. While follow-on missions can take advantage of this general 3U CubeSat platform to test the on-orbit performance of several different types of deformable mirrors, this first design accommodates a 32-actuator Boston Micromachines MEMS deformable mirror.en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (NASA Space Technology Research Fellowship)en_US
dc.description.sponsorshipMIT International Science and Technology Initiativeen_US
dc.description.sponsorshipMassachusetts Institute of Technology. Undergraduate Research Opportunities Programen_US
dc.language.isoen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.926681en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceMIT web domainen_US
dc.titleCubeSat deformable mirror demonstrationen_US
dc.typeArticleen_US
dc.identifier.citationCahoy, Kerri, Anne Marinan, Caitlin Kerr, Kezi Cheng, and Sara Jamil. “CubeSat deformable mirror demonstration.” In Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84424F-84424F-11. SPIE - International Society for Optical Engineering, 2012. © 2012 Society of Photo-Optical Instrumentation Engineers (SPIE)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Aeronautics and Astronauticsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Materials Science and Engineeringen_US
dc.contributor.mitauthorCahoy, Kerrien_US
dc.contributor.mitauthorMarinan, Anne D.en_US
dc.contributor.mitauthorKerr, Caitlin E.en_US
dc.contributor.mitauthorCheng, Kezien_US
dc.contributor.mitauthorJamil, Saraen_US
dc.relation.journalProceedings of SPIE--the International Society for Optical Engineeringen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsCahoy, Kerri; Marinan, Anne; Kerr, Caitlin; Cheng, Kezi; Jamil, Saraen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-7791-5124
dc.identifier.orcidhttps://orcid.org/0000-0001-5391-9844
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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