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Scientific Programmes with India's National Large Solar Telescope and their contribution to Prominence Research

Published online by Cambridge University Press:  06 January 2014

S. S. Hasan*
Affiliation:
Indian Institute of Astrophysics, Bangalore 560034, India email: [email protected]
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Abstract

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The primary objective of the 2-m National Large Solar Telescope (NLST) is to study the solar atmosphere with high spatial and spectral resolution. With an innovative optical design, NLST is an on-axis Gregorian telescope with a low number of optical elements and a high throughput. In addition, it is equipped with a high order adaptive optics system to produce close to diffraction limited performance.

NLST will address a large number of scientific questions with a focus on high resolution observations. With NLST, high spatial resolution observations of prominences will be possible in multiple spectral lines. Studies of magnetic fields, filament eruptions as a whole, and the dynamics of filaments on fine scales using high resolution observations will be some of the major areas of focus.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

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