Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6703
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dc.contributor.authorMurthy, J-
dc.contributor.authorRahna, P. T-
dc.contributor.authorSutaria, F. K-
dc.contributor.authorSafonova, M-
dc.contributor.authorGudennavar, S. B-
dc.contributor.authorBubbly, S. G-
dc.date.accessioned2020-11-10T02:01:24Z-
dc.date.available2020-11-10T02:01:24Z-
dc.date.issued2017-08-
dc.identifier.citationCurrent Science, Vol. 113, No. 4, pp. 616- 619en_US
dc.identifier.issn0011-3891-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6703-
dc.descriptionOpen Access © Current Science Association http://www.currentscience.ac.in/Volumes/113/04/0616.pdfen_US
dc.description.abstractThe Solar Ultraviolet Imaging Telescope (SUIT) is an instrument onboard the Aditya-L1 spacecraft, the first dedicated solar mission of the Indian Space Research Organization (ISRO), which will be put in a halo orbit at the Sun-Earth Langrage point (L1). SUIT has an off-axis Ritchey–Chrétien configuration with a combination of 11 narrow and broad bandpass filters which will be used for full-disk solar imaging in the Ultravoilet (UV) wavelength range 200-400 nm. It will provide near simultaneous observations of lower and middle layers of the solar atmosphere, namely the Photosphere and Chromosphere. These observations will help to improve our understanding of coupling and dynamics of various layers of the solar atmosphere, mechanisms responsible for stability, dynamics and eruption of solar prominences and Coronal Mass ejections, and possible causes of solar irradiance variability in the Near and Middle UV regions, which is of central interest for assessing the Sun’s influence on climate.en_US
dc.language.isoenen_US
dc.publisherCurrent Science Associationen_US
dc.subjectOxygen and ozone chemistryen_US
dc.subjectSolar radiationen_US
dc.subjectSun climate relationshipen_US
dc.subjectUltraviolet imaging telescopeen_US
dc.titleThe Solar Ultraviolet Imaging Telescope on-board Aditya-L1en_US
dc.typeArticleen_US
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