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Progress of site survey for large solar telescopes in western China

Published online by Cambridge University Press:  09 September 2016

Yu Liu
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Tengfei Song
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Xuefei Zhang
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Shunqing Liu
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Mingyu Zhao
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Zhanjun Tian
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Yuhu Miao
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Hongbo Li
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Jing Huang
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Baoyu Su
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Yongyin Lu
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Xiaobo Li
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Qiwu Song
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: [email protected]
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Abstract

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Excellent sites are necessary for developing and installing ground-based large telescopes. For very-high-resolution solar observations, it had been unclear whether there exist good candidate sites in the west areas in China, including the Tibetan Plateau and the Pamirs Plateau. The project of solar site survey for the next-generation large solar telescopes, i.e., the Chinese Giant Solar Telescope (CGST) and the large coronagraph, has been launched since 2011. Based on the close collaboration among Chinese solar society and the scientists from NSO, HAO and other institutes, we have successfully developed the standard instruments for solar site survey and applied them to more than 50 different sites distributed in Xinjiang, Tibet, Qinghai, Sichuan, Yunnan and Ningxia provinces. We have built two long-term monitoring sites in Tibet and the large Shangri-La to take systematic site data. Clear evidence, including the key parameters of seeing factor, sky brightness and water vapor content, has indicated that a few potential sites in the large Tibetan areas should obtain the excellent astronomical conditions for our purpose to develop CGST and large coronagraph. We introduce the fresh site survey results in this report.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

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