首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Color pictures of sprites from non-dedicated observation on board the International Space Station
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Color pictures of sprites from non-dedicated observation on board the International Space Station

机译:来自国际空间站非专用观测的子画面彩色图片

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Very recently NASA astronauts took a new set of pictures from the International Space Station during night time in the frame of the NASA Crew Earth Observations program, giving a new opportunity to observe in color sprites and their parent lightning flashes. During about 20 h of observations, nondirectly dedicated to thunderstorm studies, 15 sprites were observed from August 2011 to April 2012. Chromatic observations allow analyzing thoroughly the main components of the sprite radiation. The red and green emissions, observed in all the sprite images, are due to the radiation of the first positive band system of molecular nitrogen N_2. The blue emission, present in only 2 out of 15 sprites, is produced by the radiation of bands of the second positive band system of N_2 and bands of the first negative band system of N_2~+ ions. It indicates the possible presence of ionization in these two sprites. The sprite brightness is equivalent to the Jupiter one.
机译:最近,美国宇航局的宇航员在夜间利用NASA乘员组地球观测计划的框架从国际空间站拍摄了一组新照片,这为观察彩色子星及其母体闪电提供了新的机会。在2011年8月至2012年4月的约20小时非直接用于雷暴研究的观测中,观测到15个精灵。彩色观测可以彻底分析精灵辐射的主要成分。在所有子画面图像中观察到的红色和绿色发射是由于分子氮N_2的第一个正带系统的辐射引起的。在15个子图中仅2个存在的蓝色发射是由N_2的第二正带系统的能带和N_2〜+离子的第一负带系统的能带辐射产生的。它表明这两个子图中可能存在电离。精灵的亮度相当于木星之一。

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