New vacuum solar telescope and observations with high resolution

The New Vacuum Solar Telescope (NVST) is a one meter vacuum solar telescope that aims to observe fine structures on the Sun. The main goals of NVST are high resolution imaging and spectral observations, including measurements of the solar magnetic field. NVST is the primary ground-based facility use...

Full description

Saved in:
Bibliographic Details
Published inResearch in astronomy and astrophysics Vol. 14; no. 6; pp. 705 - 718
Main Authors Liu, Zhong, Xu, Jun, Gu, Bo-Zhong, Wang, Sen, You, Jian-Qi, Shen, Long-Xiang, Lu, Ru-Wei, Jin, Zhen-Yu, Chen, Lin-Fei, Lou, Ke, Li, Zhi, Liu, Guang-Qian, Xu, Zhi, Rao, Chang-Hui, Hu, Qi-Qian, Li, Ru-Feng, Fu, Hao-Wen, Wang, Feng, Bao, Men-Xian, Wu, Ming-Chan, Zhang, Bo-Rong
Format Journal Article
LanguageEnglish
Published 01.06.2014
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:The New Vacuum Solar Telescope (NVST) is a one meter vacuum solar telescope that aims to observe fine structures on the Sun. The main goals of NVST are high resolution imaging and spectral observations, including measurements of the solar magnetic field. NVST is the primary ground-based facility used by the Chinese solar research community in this solar cycle. It is located by Fuxian Lake in southwest China, where the seeing is good enough to perform high resolution observations. We first introduce the general conditions at the Fuxian Solar Observatory and the primary science cases of NVST. Then, the basic structures of this telescope and instruments are described in detail. Finally, some typical high resolution data of the solar photosphere and chromosphere are also shown.
Bibliography:telescopes -- instrumentation: adaptive optics -- instrumentation: spec-trographs -- techniques: high angular resolution -- Sun: magnetic fields
11-5721/P
The New Vacuum Solar Telescope (NVST) is a one meter vacuum solar telescope that aims to observe fine structures on the Sun. The main goals of NVST are high resolution imaging and spectral observations, including measurements of the solar magnetic field. NVST is the primary ground-based facility used by the Chinese solar research community in this solar cycle. It is located by Fuxian Lake in southwest China, where the seeing is good enough to perform high resolution observations. We first introduce the general conditions at the Fuxian Solar Observatory and the primary science cases of NVST. Then, the basic structures of this telescope and instruments are described in detail. Finally, some typical high resolution data of the solar photosphere and chromosphere are also shown.
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:1674-4527
2397-6209
DOI:10.1088/1674-4527/14/6/009