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SPACE SOLAR TELESCOPE
AI, G; Culhane, JL; Hiei, E
1995
Source PublicationSOLAR FLARE, CORONAL AND HELIOSPHERIC DYNAMICS
Volume17Issue:4/5Pages:343-354
AbstractThe 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.
Indexed ByISTP ; SCI
Language英语
WOS IDWOS:A1995BD87Y00065
Citation statistics
Cited Times:5[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8331
Collection院士
Recommended Citation
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.
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