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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7972
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dc.contributor.authorVenkata Suresh, Narra-
dc.contributor.authorPrasad, B. R-
dc.contributor.authorSingh, J-
dc.date.accessioned2022-06-30T05:22:12Z-
dc.date.available2022-06-30T05:22:12Z-
dc.date.issued2022-02-
dc.identifier.citationExperimental Astronomy, Vol. 53, No. 1, pp. 71-82en_US
dc.identifier.issn1572-9508-
dc.identifier.urihttp://hdl.handle.net/2248/7972-
dc.descriptionRestricted Accessen_US
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractOne of the unique features of Visible Emission Line Coronagraph (VELC) on board Aditya-L1 mission is spectropolarimetric observations in coronal emission line centred at 10747 Å. Spectropolarimetric observations at 10747 Å helps in understanding coronal magnetic feld topology and Line of Sight (LOS) feld strength measurements. Coronal magnetic feld measurements provide useful information about the drivers for space weather. To carry out the polarimetric observations a dual beam spectropolarimeter is employed in the VELC. Spectropolarimeter package consists of a Quarter Wave Plate (QWP), Polarizing Beam Displacer (PBD) and Half Wave Plate (HWP). Current manuscript provides an overview of the design of spectropolarimetric channel of VELC and the realization aspects.en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.urihttps://doi.org/10.1007/s10686-021-09816-7-
dc.rights© The Author(s), under exclusive licence to Springer Nature B.V. 2021-
dc.subjectVELCen_US
dc.subjectAditya-L1en_US
dc.subjectSolar coronaen_US
dc.subjectEmission linesen_US
dc.subjectSpectropolarimetryen_US
dc.subjectMagnetic fielden_US
dc.titleSpectropolarimetry package for visible emission line coronagraph (VELC) on board Aditya-L1 missionen_US
dc.typeArticleen_US
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