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首页> 外文期刊>Solar Physics >Widespread Occurrence of Trenching Patterns in the Granulation Field: Evidence for Roll Convection?
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Widespread Occurrence of Trenching Patterns in the Granulation Field: Evidence for Roll Convection?

机译:造粒场中沟槽形式的广泛发生:辊对流的证据吗?

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Time-averaged series of granulation images are analysed using COLIBRI, a purpose-adapted version of a code originally developed to detect straight or curvilinear features in aerospace images. The image-processing algorithm utilises a nonparametric statistical criterion that identifies a straight-line segment as a linear feature (lineament) if the photospheric brightness at a certain distance from this line on both sides is stochastically lower or higher than at the line itself. Curvilinear features can be detected as chains of lineaments, using a modified criterion. Once the input parameters used by the algorithm are properly adjusted, the algorithm highlights “ridges” and “trenches” in the relief of the brightness field, drawing white and dark lanes. The most remarkable property of the trenching patterns is a nearly universally present parallelism of ridges and trenches. Since the material upflows are brighter than the downflows, the alternating, parallel light and dark lanes should reflect the presence of roll convection in the subphotospheric layers. If the numerous images processed by us are representative, the patterns revealed suggest a widespread occurrence of roll convection in the outer solar convection zone. In particular, the roll systems could form the fine structure of larger scale, supergranular and/or mesogranular convection flows. Granules appear to be overheated blobs of material that could develop into convection rolls owing to instabilities of roll motion.
机译:使用COLIBRI分析时间平均系列的造粒图像,COLIBRI是最初为检测航空图像中的直线或曲线特征而开发的专用代码版本。图像处理算法利用非参数统计准则,如果在距该直线两侧一定距离处的光球亮度随机地低于或高于直线本身,则将直线段标识为线性特征(直线)。使用修改后的标准,可以将曲线特征检测为线条链。正确调整算法使用的输入参数后,算法会在亮度字段的凸显部分突出显示“山脊”和“沟槽”,绘制白色和深色车道。沟槽图案的最显着特性是几乎普遍存在的脊和沟槽的平行度。由于材料的上升流比下降的流明亮,因此交替,平行的明暗通道应反映出亚光圈层中存在滚动对流。如果我们处理的大量图像具有代表性,则揭示的模式表明在太阳对流外层普遍存在滚动对流。特别地,辊系统可以形成较大规模,超颗粒和/或中颗粒对流的精细结构。颗粒似乎是过热的团块,由于滚动运动的不稳定性而可能发展成对流辊。

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