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首页> 外文期刊>Science >HST FAR-ULTRAVIOLET IMAGING OF JUPITER DURING THE IMPACTS OF COMET SHOEMAKER-LEVY 9
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HST FAR-ULTRAVIOLET IMAGING OF JUPITER DURING THE IMPACTS OF COMET SHOEMAKER-LEVY 9

机译:彗星突击步枪等级9对木星的HST远紫外线成像

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Hubble Space Telescope far-ultraviolet images of Jupiter during the Shoemaker-Levy 9 impacts show the impact regions darkening over the 2 to 3 hours after the impact, becoming darker and more extended than at longer wavelengths, which indicates that ultraviolet-absorbing gases or aerosols are more extended, more absorbing, and at higher altitudes than the absorbers of visible light, Transient auroral emissions were observed near the magnetic conjugate point of the K impact site just after that impact. The global auroral activity was fainter than average during the impacts, and a variable auroral emission feature was observed inside the southern auroral oval preceding the impacts of fragments Q1 and Q2.
机译:在Shoemaker-Levy 9撞击期间,哈勃太空望远镜拍摄的木星远紫外线图像显示,撞击后2至3个小时,撞击区域变暗,比更长的波长更暗,且延伸范围更大,这表明吸收紫外线的气体或气溶胶与可见光的吸收剂相比,它们具有更大的扩展性,更强的吸收性和更高的海拔高度,在那次撞击之后,在K撞击点的磁共轭点附近观察到了短暂的极光发射。在撞击过程中,全球极光活动较平均值弱,并且在碎片Q1和Q2撞击之前,在南部极光椭圆形内部观测到了可变的极光发射特征。

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