Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5697
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dc.contributor.authorHasan, S. S-
dc.date.accessioned2012-02-17T11:00:01Z-
dc.date.available2012-02-17T11:00:01Z-
dc.date.issued2011-
dc.identifier.citationASI Conference Series, Vol. 2, pp. 37-45en
dc.identifier.isbn978-81-922926-0-1-
dc.identifier.urihttp://hdl.handle.net/2248/5697-
dc.descriptionOpen Accessen
dc.description.abstractThe National Large Solar Telescope NLST will be a state-ofthe- art 2-m class telescope for carrying out high-resolution studies of the solar atmosphere. Sites in the Himalayan region at altitudes greater than 4000-m that have extremely low water vapor content and are una ected by monsoons are under evaluation. This project is led by the Indian Institute of Astrophysics and has national and international partners. Its geographical location will fill the longitudinal gap between Japan and Europe and is expected to be the largest solar telescope with an aperture larger than 1.5 m till ATST and EST come into operation. NLST is an on-axis alt-azimuth Gregorian multi-purpose open telescope with the provision of carrying out night time stellar observations using a spectrograph at the final focus. The telescope utilizes an innovative design with low number of reflections to achieve a high throughput and low polarization. High order adaptive optics is integrated into the design that works with a modest Fried parameter of 7-cm to give di raction limited performance. The telescope will be equipped with a suite of post-focusen
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.rights© Astronomical Society of Indiaen
dc.subjectSun: general – telescopesen
dc.titleNational Large Solar Telescope of Indiaen
dc.typeArticleen
Appears in Collections:IIAP Publications

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