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Subsurface Vorticity of Flaring versus Flare-Quiet Active Regions

机译:扩口与扩口静区的地下涡度

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We apply discriminant analysis to 1023 active regions and their subsurface-flow parameters, such as vorticity and kinetic helicity density, with the goal of distinguishing between flaring and non-flaring active regions. We derive synoptic subsurface flows by analyzing GONG high-resolution Doppler data with ring-diagram analysis. We include magnetic-flux values in the discriminant analysis derived from NSO Kitt Peak and SOLIS synoptic maps binned to the same spatial scale as the helioseismic analysis. For each active region, we determine the flare information from GOES and include all flares within 60° central meridian distance to match the coverage of the ring-diagram analysis. The subsurface-flow characteristics improve the ability to distinguish between flaring and non-flaring active regions. For the C- and M-class flare category, the most important subsurface parameter is the so-called structure vorticity, which estimates the horizontal gradient of the horizontal-vorticity components. The no-event skill score, which measures the improvement over predicting that no events occur, reaches 0.48 for C-class flares and 0.32 for M-class flares, when the structure vorticity at three depths combined with total magnetic flux are used. The contributions come mainly from shallow layers within about 2 Mm of the surface and layers deeper than about 7 Mm.
机译:我们将判别分析应用于1023个活动区域及其地下流动参数,例如涡度和动力学螺旋密度,目的是区分扩口活动区域和非扩口活动区域。我们通过使用环形图分析来分析GONG高分辨率多普勒数据,从而得出天气事件的地下流量。我们在判别分析中包括磁通量值,这些判别分析源自NSO基特峰和SOLIS天气图,这些图被装箱到与日震分析相同的空间比例。对于每个活动区域,我们从GOES确定耀斑信息,并包括60°中心子午线距离内的所有耀斑,以匹配环图分析的覆盖范围。地下流动特征提高了区分扩口和非扩口活性区域的能力。对于C级和M级耀斑类别,最重要的地下参数是所谓的结构涡度,它估计水平涡度分量的水平梯度。当使用三个深度的结构涡度并结合总磁通量时,无事件技能得分(用于衡量对预测没有事件发生的改善),对C类耀斑为0.48,对M类耀斑为0.32。贡献主要来自表面约2 Mm内的浅层和深于约7 Mm的层。

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