EUV observations of the solar corona with superhigh spatial resolution in the ARCA project
EUV observations of the solar corona with superhigh spatial resolution in the ARCA project
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ARCA 项目中对日冕进行超高空间分辨率的 EUV 观测
DOI：
10.3103/s1062873811010163
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发表时间：
2011
影响因子：
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通讯作者：
A. Ulyanov
中科院分区：
文献类型：
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作者：
S. Kuzin;S. Bogachev;A. Pertsov;S. Shestov;A. Reva;A. Ulyanov
以亚秒级的空间分辨率观测太阳的热日冕对于解决一些基本的太阳物理学问题具有重要意义。俄罗斯科学院列别捷夫物理研究所正在开发的新ARCA卫星观测站将首先提供空间分辨率约为0.18角秒的热日冕图像。讨论了天文台的科学和技术特点。
Observing the Sun’s hot corona with sub-second spatial resolution is important in solving a number of basic solar physics problems. The new ARCA satellite observatory under development at the Lebedev Physical Institute, Russian Academy of Sciences, will be first to provide images of the hot solar corona with a spatial resolution of about 0.18 arcsec. Scientific and technical features of the observatory are discussed.