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IUE's View of Callisto: Detection of an SO2 Absorption Correlated to Possible Torus Neutral Wind Alterations

机译:IUE的Callisto观点:检测与可能的环面中性风变化相关的SO2吸收

摘要

Observations taken with the International Ultraviolet Explorer (IUE) detected a 0.28 micron absorption feature on Callisto's leading and Jupiter-facing hemispheres. This feature is similar to Europa's 0.28 micron feature, however it shows no correlation with magnetospheric ion bombardment. The strongest 0.28 micron signature is seen in the region containing the Valhalla impact. This absorption feature also shows some spatial correlation to possible neutral wind interactions, suggestive of S implantation (rather than S(sub x)) into Callisto's water ice surface, Indications of possible temporal variations (on the 10% level) are seen at other wavelengths between the 1984-1986 and the 1996 observations.
机译:使用国际紫外线探测器(IUE)进行的观察发现,在Callisto的前半球和面对木星的半球上有0.28微米的吸收特征。此功能类似于Europa的0.28微米功能,但与磁层离子轰击无关。在包含瓦尔哈拉撞击的区域中看到了最强的0.28微米标记。这种吸收特征还显示出与可能的中性风相互作用存在一定的空间相关性,暗示着将S注入(而不是S(sub x))注入Callisto的水冰表面,并在其他波长下看到了可能的时间变化(在10%的水平) 1984年至1986年至1996年的观测值之间。

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