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From NVST to CGST
文献类型：会议论文
| 作者 | Liu Z(刘忠)
|
| 出版日期 | 2014-10 |
| 会议名称 | 7th Solar Polarization Workshop (SPW7) |
| 会议日期 | 2013-09-09 |
| 会议地点 | Kunming, PEOPLES R CHINA |
| 卷号 | 489 |
| 页码 | 247-262 |
| 英文摘要 | The New Vacuum Solar Telescope (NVST) is a 1 m vacuum solar telescope. The main tasks of NVST are high resolution imaging and spectral observations, including the measurements of solar magnetic field. The Chinese Giant Solar Telescope (CGST) is the next generation ground-based solar telescope proposed by Chinese solar community. The differences between NVST and CGST are not only the differences of performance parameters but also the differences of science goals and the differences in design concepts. In this paper, the information of NVST and CGST are first introduced, including the science goals, the basic structures and typical instruments. Then, the general design principles of the next generation large solar telescope are discussed based on the comparisons and analyses. |
| 收录类别 | CPCI |
| 产权排序 | 第一完成单位 |
| 会议网址 | http://adsabs.harvard.edu/abs/2014ASPC..489..247L |
| 会议录 | Astronomical Society of the Pacific (ASP) Conference Series - SOLAR POLARIZATION 7
 |
| 会议录出版者 | ASTRONOMICAL SOC PACIFIC |
| 学科主题 | Astronomy & Astrophysics |
| 会议录出版地 | 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA |
| 语种 | 英语 |
| ISBN号 | 978-1-58381-863-3; 978-1-58381-862-6 |
| WOS记录号 | WOS:000370308600024 |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9657]  |
| 专题 | 云南天文台_抚仙湖太阳观测站 |
| 作者单位 | Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, China |
| 推荐引用方式 GB/T 7714 | Liu Z. From NVST to CGST[C]. 见:7th Solar Polarization Workshop (SPW7). Kunming, PEOPLES R CHINA. 2013-09-09.http://adsabs.harvard.edu/abs/2014ASPC..489..247L. |
入库方式： OAI收割
来源：云南天文台
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