Science. 1995 Jun 16;268(5217):1598-601. doi: 10.1126/science.268.5217.1598.
Röntgensatellit (ROSAT) observations made shortly before and during the collision of comet Shoemaker-Levy 9 with Jupiter show enhanced x-ray emissions from the planet's northern high latitudes. These emissions, which occur at System III longitudes where intensity enhancements have previously been observed in Jupiter's ultraviolet aurora, appear to be associated with the comet fragment impacts in Jupiter's southern hemisphere and may represent brightenings of the jovian x-ray aurora caused either by the fragment impacts themselves or by the passage of the fragments and associated dust clouds through Jupiter's inner magnetosphere.
罗森卫星(ROSAT)在苏梅克-列维 9 号彗星与木星碰撞前后进行的观测显示,木星的高纬度地区发出了增强的 X 射线辐射。这些辐射出现在太阳系 III 经度上,此前在木星的紫外极光中已经观察到强度增强,它们似乎与木星南半球的彗星碎片撞击有关,可能代表了木星 X 射线极光的增亮,这可能是由碎片撞击本身或碎片和相关尘埃云通过木星内部磁层引起的。