SPACE SOLAR TELESCOPE
文献类型：期刊论文
| 作者 | AI, G ; Culhane, JL; Hiei, E
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| 刊名 | SOLAR FLARE, CORONAL AND HELIOSPHERIC DYNAMICS
 |
| 出版日期 | 1995 |
| 卷号 | 17期号:4/5页码:343-354 |
| 英文摘要 | The Space has idea observing conditions of astronomy: observable in ail wavelengths; continuous temporal coverage; observable in all direction; avoid disturbances produced by the atmosphere (seeing and stray light); super coherence length and so on. Following the space technology is developed further, it is not slightly doubt that space astronomy will become the major part of the astronomy. The solar magnetic fields provide the major incentive to do solar physics. The small spatial extent of the magnetically constrained structures and processes in the solar atmosphere provide the major incentive for high resolution solar telescope. The super high spatial resolution, the visibility of the out solar atmosphere in the ultraviolet and X-ray domains, and continuous evolution study provide the major incentive for space solar observation. |
| 收录类别 | ISTP ; SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:A1995BD87Y00065 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/8331]  |
| 专题 | 国家天文台_院士 |
| 推荐引用方式 GB/T 7714 | AI, G,Culhane, JL,Hiei, E. SPACE SOLAR TELESCOPE[J]. SOLAR FLARE, CORONAL AND HELIOSPHERIC DYNAMICS,1995,17(4/5):343-354. |
| APA | AI, G,Culhane, JL,&Hiei, E.(1995).SPACE SOLAR TELESCOPE.SOLAR FLARE, CORONAL AND HELIOSPHERIC DYNAMICS,17(4/5),343-354. |
| MLA | AI, G,et al."SPACE SOLAR TELESCOPE".SOLAR FLARE, CORONAL AND HELIOSPHERIC DYNAMICS 17.4/5(1995):343-354. |
入库方式： OAI收割
来源：国家天文台
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