卡西尼号紫外可见光谱仪 2017 年对土星上的恩克拉多斯极光足迹的观测

W. Pryor, Fabiola P. Magalhães, Laurent Lamy, R. Prangé, Larry W. Esposito, J. Gustin, A. Rymer, A. Sulaiman
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摘要

紫外线成像摄谱仪(UVIS)的观测结果显示,2017年9月14日,在卡西尼号任务即将结束时,土星上出现了恩克拉多斯极光足迹。通过缓慢回转卡西尼号航天器,使其与紫外成像分光仪长狭缝成直角,获得了一系列土星北极极光图像。对这些图像进行了边缘拟合,以改进航天器的几何形状。在近 4 小时的五幅连续图像上,我们看到了由于电子撞击原子和分子氢而产生的 88-118 nm 波长的极紫外通道发射增强,这正是预计的土卫二极光足迹位置。在同时获得的远紫外 111-165 nm 波长图像中,至少有两幅图像的发射增强,具有极光发射的预期光谱特征。虽然大多数卡西尼紫外可见光极光图像都没有显示出恩克拉多斯极光足迹,但这些2017年的图像支持了早先在2008年卡西尼紫外可见光可见光数据中探测到的土星上与恩克拉多斯有关的光斑。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Cassini UVIS Observations of the Enceladus Auroral Footprint on Saturn in 2017
Ultraviolet Imaging Spectrograph (UVIS) observations show the Enceladus auroral footprint on Saturn on 2017 September 14, near the end of the Cassini mission. A series of Saturn north polar auroral images were obtained by slowly slewing the Cassini spacecraft at right angles to the UVIS long slit. The images were limb-fit to improve the spacecraft geometry. Enhanced extreme-ultraviolet 88–118 nm channel emissions due to electron impact on atomic and molecular hydrogen were seen in the expected location for the Enceladus auroral footprint on five successive images spanning almost 4 hr. Enhanced emissions were also seen in simultaneously obtained far-ultraviolet 111–165 nm images in at least two of these images, with the spectral signature expected for auroral emissions. While most Cassini UVIS auroral images do not show the Enceladus auroral footprint, these 2017 images support the earlier detection of an Enceladus-linked spot on Saturn in 2008 Cassini UVIS data.
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