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An Annular Eclipse on May 31,2003, Observed in Extreme Ultraviolet

机译:2003年5月31日的环形月食,用极紫外观测

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The CORONAS-F spacecraft crossed the zone of the ring solar eclipse three times on May 31,2003. A considerable decrease in solar radiation was detected by the spacecraft instruments for these moments. The passages through the eclipse zone were registered by the VUSS instrument, which measured the shortwave solar radiation flux near the hydrogen Lyman alpha line, and by the DIFOS instrument, which was sensitive to infrared, visible, and near-ultraviolet radiation. The eclipse is also clearly seen in solar images obtained by the X-ray SPIRIT telescope. Some details of measurement results are discussed.
机译:2003年5月31日,CORONAS-F航天器三度越过环形日食区。在这些时刻,航天器仪器检测到太阳辐射明显下降。通过月蚀区的通道由VUSS仪器和DIFOS仪器记录,该仪器测量氢Lymanα线附近的短波太阳辐射通量,而DIFOS仪器对红外,可见光和近紫外线辐射敏感。在X射线SPIRIT望远镜获得的太阳图像中也可以清楚看到日食。讨论了测量结果的一些细节。

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