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首页> 外文期刊>Planetary and space science >Dynamics of Saturn's magnetodisk near Titan's orbit: Comparison of Cassini magnetometer observations from real and virtual Titan flybys
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Dynamics of Saturn's magnetodisk near Titan's orbit: Comparison of Cassini magnetometer observations from real and virtual Titan flybys

机译:土星磁场在土卫六轨道附近的动力学:卡西尼号磁力计从真实和虚拟土卫六飞越观测的比较

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摘要

We analyze the variability of the ambient magnetospheric field along Titan's orbit at 20.3 Saturn radii. However, while our preceding study (Simon et al., 2010) focused on Cassini magnetometer observations from the 62 Titan flybys (TA-T62) between October 2004 and October 2009, the present work discusses magnetic field data that were collected near Titan's orbit when the moon was far away. In analogy to the observations during TA-T62, the magnetospheric fields detected during these 79 "virtual" Titan flybys are strongly affected by the presence of Saturn's bowl-shaped and highly dynamic magnetodisk current sheet. We therefore provide a systematic classification of the magnetic field observations as magnetodisk current sheet or lobe-type scenarios. Among the 141 (62 real+79 virtual) crossings of Titan's orbit between July 2004 and December 2009, only 17 encounters (9 real+8 virtual) took place within quiet, magnetodisk lobe-type fields. During another 50 encounters (21 real + 29 virtual), rapid transitions between current sheet and lobe fields were observed around the moon's orbital plane. Most of the encounters (54 = 22 real+32 virtual) occurred when Titan's orbit was embedded in highly distorted current sheet fields, thereby invalidating the frequently applied idealized picture of Titan interacting with a homogeneous and stationary magnetospheric background field. The locations of real and virtual Titan flybys are correlated to each other. Each of the 62 real Titan flybys possesses at least one virtual counterpart that occurred shortly before or after the real encounter and at nearly the same orbital position. A systematic comparison between Cassini magnetometer observations from the real Titan flybys and their virtual companions suggests that there is no clear evidence of Titan exerting a significant level of control on the vertical oscillatory motion of the magnetodisk near its orbit.
机译:我们分析了土星半径为20.3的土卫六磁场沿泰坦轨道的变化。然而,虽然我们先前的研究(Simon等,2010)集中于2004年10月至2009年10月之间从62颗泰坦飞掠物(TA-T62)进行的卡西尼磁力计观测,但本研究讨论了在泰坦轨道附近收集的磁场数据。月亮很远。与TA-T62期间的观测结果类似,在这79次“虚拟”泰坦飞越中检测到的磁层场受到土星碗形且高度动态的磁盘电流片的强烈影响。因此,我们提供了磁场观测的系统分类,如磁盘当前工作表或叶状方案。在2004年7月至2009年12月,泰坦轨道的141次(62实+ 79虚拟)穿越中,只有17次相遇(9实+ 8虚拟)跨越了安静的磁极瓣型场。在另外50次相遇中(21个真实+ 29个虚拟),在月球轨道平面周围观察到了当前表层和波瓣场之间的快速过渡。大多数遭遇(54 = 22实+ 32虚拟)是在土卫六的轨道嵌入高度扭曲的当前工作表磁场中时发生的,从而使经常使用的理想化的土卫六与均匀且静止的磁层背景场相互作用的理想图像无效。真实和虚拟Titan掠过的位置相互关联。 62个真实的泰坦飞越中的每一个都拥有至少一个虚拟的对应物,该对应物在真实相遇之前或之后不久发生,并且处于几乎相同的轨道位置。从实际的土卫六飞掠者和他们的虚拟伴星进行的卡西尼磁力计观测结果之间的系统比较表明,没有明显的证据表明土卫六对磁碟在其轨道附近的垂直振荡运动施加了重要的控制作用。

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