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首页> 外文期刊>Icarus: International Journal of Solar System Studies >A predator-prey model for moon-triggered clumping in Saturn's rings
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A predator-prey model for moon-triggered clumping in Saturn's rings

机译:土星环中的月球触发团块的捕食者-猎物模型

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摘要

UVIS occultation data show clumping in Saturn's F ring and at the B ring outer edge, indicating aggregation and disaggregation at these locations that are perturbed by Prometheus and by Mimas. The inferred timescales range from hours to months. Occultation profiles of the edge show wide variability, indicating perturbations by local mass aggregations. Structure near the B ring edge is seen in power spectral analysis at scales 200-2000. m. Similar structure is also seen at the strongest density waves, with significance increasing with resonance strength. For the B ring outer edge, the strongest structure is seen at longitudes 90° and 270° relative to Mimas. This indicates a direct relation between the moon and the ring clumping. We propose that the collective behavior of the ring particles resembles a predator-prey system: the mean aggregate size is the prey, which feeds the velocity dispersion; conversely, increasing dispersion breaks up the aggregates. Moons may trigger clumping by streamline crowding, which reduces the relative velocity, leading to more aggregation and more clumping. Disaggregation may follow from disruptive collisions or tidal shedding as the clumps stir the relative velocity. For realistic values of the parameters this yields a limit cycle behavior, as for the ecology of foxes and hares or the " boom-bust" economic cycle. Solving for the long-term behavior of this forced system gives a periodic response at the perturbing frequency, with a phase lag roughly consistent with the UVIS occultation measurements. We conclude that the agitation by the moons in the F ring and at the B ring outer edge drives aggregation and disaggregation in the forcing frame. This agitation of the ring material may also allow fortuitous formation of solid objects from the temporary clumps, via stochastic processes like compaction, adhesion, sintering or reorganization that drives the denser parts of the aggregate to the center or ejects the lighter elements. Any of these more persistent objects would then orbit at the Kepler rate. We would also expect the formation of clumps and some more permanent objects at the other perturbed regions in the rings... including satellite resonances, shepherded ring edges, and near embedded objects like Pan and Daphnis (where the aggregation/disaggregation cycles are forced similar to Prometheus forcing of the F ring).
机译:UVIS的掩星数据表明,土星的F环和B环的外边缘有团块,表明这些位置的聚集和分解受到普罗米修斯和米玛斯的干扰。推断的时间范围从数小时到数月不等。边缘的掩星剖面显示出很大的变化性,表明局部质量聚集引起的扰动。在200-2000的功率谱分析中可以看到B环边缘附近的结构。米在最强的密度波上也可以看到类似的结构,其重要性随着共振强度的增加而增加。对于B环外缘,相对于Mimas在90°和270°的经度处看到最坚固的结构。这表明月亮和环结块之间存在直接关系。我们提出,环粒子的集体行为类似于一个捕食者-被捕食者系统:平均聚集体大小是被捕食者,它为速度分散提供了动力;相反,增加分散度会破坏聚集体。卫星可能会因流线型拥挤而触发结块,从而降低相对速度,从而导致更多的聚集和结块。当团块搅动相对速度时,破坏性碰撞或潮汐脱落可能导致分解。对于参数的实际值,这会产生极限循环行为,例如狐狸和野兔的生态状况或“繁荣-萧条”经济周期。解决此强制系统的长期行为,可在扰动频率下产生周期性响应,其相位滞后与UVIS掩星测量结果大致一致。我们得出结论,卫星在F环和B环外缘的搅动推动了强迫框架中的聚集和解聚。环材料的这种搅动还可以允许通过临时过程(例如压实,粘附,烧结或重组)从临时团块偶然形成固体,这些过程将聚集体的较密部分驱动到中心或弹出较轻的元素。这些持久性物体中的任何一个然后都将以开普勒速率旋转。我们还期望在环的其他受扰区域形成团块和一些更永久的对象……包括卫星共振,牧羊人的环形边缘以及靠近诸如Pan和Daphnis之类的嵌入式对象(聚集/分解周期被迫类似到普罗米修斯强迫F环)。

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