Propagation “over the horizon” of Saturn's radio lightning studied by three-dimensional ray tracing

A.-L. Gautier, B. Cecconi, P. Zarka, G. Fischer
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Abstract

Saturn Electrostatic Discharges (SED] are radio signature of lightning flashes originating from Saturns cloud systems. Observations of SED show that the radio horizon is larger than the visible one, especially when Cassini is in Saturns morning side (“over the horizon” effect]. Moreover, both apparition and disappearance of bursts appear to be frequency-dependent. We built a 3D ray tracing code, which computes the path propagation of radio waves through a realistic model of Saturns ionosphere, where electron density varies with local time, and were able to reproduce the typical dynamic spectrum of observed “over the horizon” events.
通过三维射线追踪研究了土星射电闪电的“超越地平线”传播
土星静电放电(SED)是源自土星云系统的闪电的无线电信号。SED的观测表明,射电视界比可见视界大,特别是当卡西尼号在土星的早晨侧时(“越过视界”效应)。此外,爆发的出现和消失似乎都与频率有关。我们建立了一个3D光线追踪代码,通过一个真实的土星电离层模型计算无线电波的传播路径,其中电子密度随当地时间的变化而变化,并能够重现观测到的“超视界”事件的典型动态光谱。
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