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首页> 外文期刊>Astronomy and astrophysics >The June 2012 transit of Venus - Framework for interpretation of observations
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The June 2012 transit of Venus - Framework for interpretation of observations

机译:金星的2012年6月过境-观测解释框架

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Context. On 5–6 June 2012 ground-based observers have the last opportunity of the century to watch the passage of Venus across the solar disk from Earth. Venus transits have traditionally provided unique insight into the Venus atmosphere through the refraction halo that appears at the planet’s outer terminator near ingress/egress. Much more recently, Venus transits have attracted renewed interest because the technique of transits is being successfully applied to the characterization of extrasolar planet atmospheres. Aims. The current work theoretically investigates the interaction of sunlight and the Venus atmosphere through the full range of transit phases, as observed from Earth and from a remote distance. Our model predictions quantify the relevant atmospheric phenomena, thereby assisting the observers of the event in the interpretation of measurements and extrapolation to the exoplanet case. Methods. Our approach relies on numerical integration of the radiative transfer equation, and includes refraction, multiple scattering, atmospheric extinction, and solar limb darkening, as well as an up-to-date description of the Venus atmosphere. Results. We produce synthetic images of the planet’s terminator during ingress/egress that demonstrate the evolving shape, brightness, and chromaticity of the halo. Our simulations reveal the impact of micrometer-sized aerosols borne in the upper haze layer of the atmosphere on the halo’s appearance. Guidelines are offered for the investigation of the planet’s upper haze from vertically-unresolved photometric measurements. In this respect, the comparison with measurements from the 2004 transit appears encouraging. We also show integrated lightcurves of the Venus-Sun system at various phases during transit and calculate the respective Venus-Sun integrated transmission spectra. The comparison of the model predictions to those for a Venus-like planet free of haze and clouds (and therefore a closer terrestrial analog) complements the discussion and sets the conclusions into a broader perspective.
机译:上下文。在2012年6月5日至6日,地面观测者将有一个世纪来最后一次机会,观看金星从地球越过太阳圆盘的过程。传统上,金星凌日通过折射晕出现在金星大气层上,该折射晕出现在行星入口/出口附近的外层终结者处。最近,金星过境引起了新的兴趣,因为过境技术已成功地用于表征太阳系外行星大气。目的从地球和远距离观察到,目前的工作理论上研究了整个过渡阶段太阳光和金星大气之间的相互作用。我们的模型预测可以量化相关的大气现象,从而帮助事件的观察者解释测量结果并推断到系外行星的情况。方法。我们的方法依赖于辐射传递方程的数值积分,包括折射,多次散射,大气消光和太阳肢体变黑,以及对金星大气的最新描述。结果。我们在进/出过程中生成行星终结者的合成图像,以显示光环的形状,亮度和色度的变化。我们的模拟揭示了大气的上层雾霾层中所携带的微米级气溶胶对光晕外观的影响。提供了从垂直方向未解决的光度测量研究行星上层雾度的指南。在这方面,与2004年的测量结果进行比较似乎令人鼓舞。我们还显示了金星-太阳系在运输过程中各个阶段的积分光曲线,并计算了各自的金星-太阳系积分透射光谱。将模型预测与没有雾霾和云的类似金星的行星(因此也有更接近的地球类似物)的模型预测进行比较,可以补充讨论并为更广阔的视野提供结论。

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