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Science with Large Solar Telescopes: Overview of SpS 6

Published online by Cambridge University Press:  05 March 2015

Gianna Cauzzi ,
Alexandra Tritschler  and
Yuanyong Deng
Gianna Cauzzi
Affiliation:
INAF-Ossevatorio Astrofisico di Arcetri, Firenze, Italy, email: gcauzzi@arcetri.astro.it
Alexandra Tritschler
Affiliation:
National Solar Observatory, Sunspot, NM 88349, USA, email: ali@nso.edu
Yuanyong Deng
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, China, email: dyy@nao.cas.cn
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Abstract

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With several large aperture optical and IR telescopes just coming on-line, or scheduled for the near future, solar physics is on the verge of a quantum leap in observational capabilities. An efficient use of such facilities will require new and innovative approaches to both observatory operations and data handling.

This two-days long Special Session discussed the science expected with large solar telescopes, and started addressing the strategies necessary to optimize their scientific return. Cutting edge solar science as derived from state-of-the-art observations and numerical simulations and modeling was presented, and discussions were held on the role of large facilities in satisfying the demanding requirements of spatial and temporal resolution, stray-light correction, and spectro-polarimetric accuracy. Building on the experience of recently commissioned telescopes, critical issues for the development of future facilities were discussed. These included operational issues peculiar to large telecopes as well as strategies for their best use.

Keywords

telescopestechniques: image processingtechniques: polarimetricmethods: numericalSun: atmospheremagnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 439 - 470
Copyright
Copyright © International Astronomical Union 2015 

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