Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8376
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dc.contributor.authorVenkata Suresh, Narra-
dc.contributor.authorHegde, Bhavana-
dc.contributor.authorDasamantarao, Utkarsha-
dc.contributor.authorSomasundaram, P. K-
dc.contributor.authorKamath, P. U-
dc.contributor.authorPrasad, B. R-
dc.date.accessioned2024-03-22T09:15:58Z-
dc.date.available2024-03-22T09:15:58Z-
dc.date.issued2023-12-
dc.identifier.citationJournal of Astronomical Instrumentation, Vol. 12, No. 4, 2350011en_US
dc.identifier.issn2251-1717-
dc.identifier.urihttp://hdl.handle.net/2248/8376-
dc.descriptionRestricted Accessen_US
dc.description.abstractVisible Emission Line Coronagraph (VELC) is the prime payload on board Aditya-L1 mission. One of the unique capabilities of VELC is the coronal magnetic field measurements from space. To achieve this, VELC performs dual beam spectropolarimetric observations in coronal emission line centered at 10747Å. Spectropolarimetric channel of VELC consists of different polarimetric components such as quarter waveplate (QWP), polarising beam displacer (PBD) and half waveplate (HWP). Calibration of individual components is essential to ensure that they meet the performance requirements of the payload. This work discusses the details of the calibration tests carried out to evaluate the performance of different polarimetric components of VELC and the results obtained.en_US
dc.language.isoenen_US
dc.publisherWorld Scientific Publishing Companyen_US
dc.relation.urihttps://doi.org/10.1142/S2251171723500113-
dc.rights© World Scientific Publishing Company-
dc.subjectSpectropolarimetryen_US
dc.subjectVELCen_US
dc.subjectSolar coronaen_US
dc.subjectAditya L1en_US
dc.subjectCoronal magnetic fieldsen_US
dc.subjectCalibrationen_US
dc.titleCalibration of Spectropolarimetry package for Visible Emission Line Coronagraph (VELC) on board Aditya-L1 missionen_US
dc.typeArticleen_US
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