Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7746
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dc.contributor.authorPruthvi, Suryadevara-
dc.date.accessioned2021-06-28T12:47:54Z-
dc.date.available2021-06-28T12:47:54Z-
dc.date.issued2019-07-
dc.identifier.citationM. Tech Thesis, University of Calcutta, Kolkataen_US
dc.identifier.urihttp://hdl.handle.net/2248/7746-
dc.descriptionThesis Supervisor B.Raghavendra Prasaden_US
dc.description.abstractAditya-L1, India’s first mission with multiple science payloads is designed to study the solar dynamics. Aditya-L1 includes multiple payloads, the significant one being the Visible Emission Line Coronagraph (VELC). VELC is designed to study the solar corona from 1.05 Ro to 3R, which has never been achieved by any other space solar mission. It consists of four channels for observation, two spectroscopic, one spectropolarimetric and one imaging channel. VELC contains 38 optical elements including mirrors, lenses, diffraction grating, etc. These 38 optical elements are made into 17 optical assemblies. The performance of each of the elements must be tested and calibrated before they can be used in the payload. This report will go through all the procedures followed for calibration of polarization modulators, polarizing beam displacers and diffraction grating.en_US
dc.language.isoenen_US
dc.publisherIndian Institute of Astrophysicsen_US
dc.rights© Indian Institute of Astrophysics-
dc.titleCalibration of subsystems of visible emission line coronagraphen_US
dc.typeThesisen_US
Appears in Collections:Integrated M.Tech-Ph.D (Tech.)

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