Magnetic flux emerges on the Sun on many different scales, from weak intranetwork to network concentrations and (ephemeral) active regions. Methods previously developed to recognize regions of magnetic emergence on MDI Full Disk magnetograms fail when applied to Hinode/SOT Stokes maps: the resolution is so much higher that simple bipoles on MDI are observed as collections of fragments. We present a new method for the automatic detection and characterization of flux emergence on a range of scales.
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机译：磁通量在许多不同的尺度上出现在太阳上，从弱的内部工作到网络浓度和（短暂的）有源区。在应用于Hinode / SOT Stokes地图时，以前开发出识别MDI全磁盘磁彩图的磁出现区域的方法：分辨率越高，MDI上的简单Bipoles被观察为片段的集合。我们提出了一种新方法，用于在一系列秤上自动检测和表征助焊剂。
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