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Proposed National Large Solar Telescope

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dc.contributor.author Singh, J
dc.date.accessioned 2007-07-27T09:02:31Z
dc.date.available 2007-07-27T09:02:31Z
dc.date.issued 2008-06
dc.identifier.citation Journal of Astrophysics & Astronomy, Vol. 29, No. 1 - 2, pp. 345 - 351 en
dc.identifier.uri http://hdl.handle.net/2248/1758
dc.description.abstract Sun’s atmosphere is an ideal place to study and test many magnetohydrodynamic (MHD) processes controlling turbulent plasma. We wish to resolve some of the finest solar features (which remain unresolved presently) and study their dynamics. Indian Institute of Astrophysics has proposed to design, fabricate and install a 2-meter class solar telescope at a suitable site in India to resolve features on the Sun of the size of about 0.1 arcsec. The focal plane instruments will include a high resolu-tion polarimeteric package to measure polarization with an accuracy of 0.01 per cent; a high spectral resolution spectrograph to obtain spectra in 5 widely separated absorption lines simultaneously and high spatial resolu-tion narrow band imagers in various lines. The Himalayan region appears to be a good choice keeping in view the prevailing dry and clear weather conditions. We have started detailed analysis of the weather conditions in the area and at some other locations in India. The site characterization will be done using the Sun-photometer, S-DIMM and SHABAR techniques to determine the seeing conditions en
dc.format.extent 1455414 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Indian Academy of Sciences en
dc.relation.uri http://www.ias.ac.in/jaa/marjun2008/absmarjun2008.html#jaa43 en
dc.subject Solar telescope en
dc.subject adaptive optics en
dc.subject spectropolarimetry—location
dc.title Proposed National Large Solar Telescope en
dc.type Article en


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