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欧空局在苏梅克-列维 9 号彗星撞击木星期间对木星的观测

EUVE Observations of Jupiter During the Impact of Comet Shoemaker-Levy 9.

出版信息

Science. 1995 Jun 16;268(5217):1595-7. doi: 10.1126/science.268.5217.1595.

Abstract

The Extreme Ultraviolet Explorer (EUVE) satellite conducted extensive observations of the jovian system before, during, and after the impact of the fragments of comet Shoemaker-Levy 9 in July 1994. About 2 to 4 hours after the impacts of several of the larger fragments, the brightness of the neutral helium (He I) resonance line at 58.4 nanometers temporarily increased by a factor of about 10. The transient 58.4-nanometer brightenings are most simply explained by resonant scattering of sunlight from the widespread high-altitude remnants of the larger impact plumes. Other possible sources of emission, such as electron impact excitation of He or radiative recombination of He(+), may contribute to the observed signal.

摘要

极紫外线探测卫星(EUVE)在 1994 年 7 月苏梅克-列维 9 号彗星碎片撞击木星系统之前、期间和之后进行了广泛的观测。在几个较大碎片撞击后大约 2 到 4 小时,58.4 纳米中性氦(He I)共振线的亮度暂时增加了约 10 倍。最合理的解释是,阳光从较大撞击羽流的广泛高空残余物中进行共振散射,导致了这种短暂的 58.4 纳米亮度增强。其他可能的发射源,如 He 的电子碰撞激发或 He(+)的辐射复合,也可能对观测到的信号有贡献。

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