首页> 外文会议>International Solar Cycles Studies symposium on solar variability as an input to the Earth's environment >INVESTIGATION OF ABSORPTION OF SOLAR EUV-RADIATION IN THE EARTH'S ATMOSPHERE AT ALTITUDES OF 100-500 KM USING SOLAR IMAGES IN THE EXPERIMENTS TEREK-C (CORONAS-Ⅰ) AND SPIRIT (CORONAS-F)
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INVESTIGATION OF ABSORPTION OF SOLAR EUV-RADIATION IN THE EARTH'S ATMOSPHERE AT ALTITUDES OF 100-500 KM USING SOLAR IMAGES IN THE EXPERIMENTS TEREK-C (CORONAS-Ⅰ) AND SPIRIT (CORONAS-F)

机译:在实验中的太阳能图像在100-500公里的海拔地球大气层中太阳能EUV - 辐射的吸收调查(Coronas-Ⅰ)和精神(Coronas-F)

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The results of measurements of absorption of solar EUV-radiation in the Earth's high atmosphere (100-500 km) using solar images obtained in occultation mode with the TEREK-C telescope on-board the Coronas-Ⅰ satellite (1994) and with the SPIRIT telescope/ spectroheliograph on-board the Coronas-F satellite (launched in 2001) are presented. Use of high resolution attenuated solar EUV images recorded in presence of absorption instead of a total flux from the whole Sun allows to determine attenuation height profiles with an accuracy better than 1 km. Possible effects of geomagnetic activity on EUV-absorption data are discussed.
机译:在地球高气氛(100-500km)中使用掩星模型中获得的太阳能图像吸收太阳能EUV辐射的测量结果与Corona-Ⅰ卫星(1994)和精神一起使用的洞穴模式。望远镜/光谱仪在核心卫星(在2001年推出)。使用高分辨率减弱的太阳能EUV图像在存在的情况下记录而不是来自整个阳光的总通量允许确定衰减高度曲线,精度优于1公里。讨论了地磁活动对EUV吸收数据的可能影响。

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