Solar dynamics imaging system a back-end instrument for the proposed NLST

dc.contributor.author	Ramesh, K. B
dc.contributor.author	Vasantharaju, N
dc.contributor.author	Hemanth, P
dc.contributor.author	Reardon, K
dc.date.accessioned	2020-11-17T12:01:55Z
dc.date.available	2020-11-17T12:01:55Z
dc.date.issued	2016-12
dc.identifier.citation	Experimental Astronomy, Vol. 42, No. 3, pp. 271-283	en_US
dc.identifier.issn	1572-9508
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7074
dc.description	Restricted Access © Springer The original publication is available at springerlink.com http://dx.doi.org/10.1007/s10686-016-9509-y	en_US
dc.description.abstract	The Solar Dynamics Imaging System (SDIS) will be one of the focal plane instruments operated at the National Large Solar Telescope (NLST). The prime objective of the instrument is to obtain high spatial and temporal resolution images of the region of interest on the Sun in the wavelength range from 390 nm to 900 nm. The SDIS provides filtergrams using broad-band filters while preserving the Strehl ratio provided by the telescope. Furthermore, the SDIS is expected to provide observations that allow image reconstruction to extract wave front information and achieve a homogenous image quality over the entire FOV.	en_US
dc.language.iso	en	en_US
dc.publisher	Springer	en_US
dc.subject	Solar	en_US
dc.subject	Broad band imaging	en_US
dc.subject	NLST	en_US
dc.title	Solar dynamics imaging system a back-end instrument for the proposed NLST	en_US
dc.type	Article	en_US