Structural Properties of Photospheric Magnetic Fields

9309901 Lawrence Digital，将使用现代分形、小波变换和渗流方法对在高空间分辨率下获得的视线太阳磁场和速度场的光度图像进行分析。这项研究将开发一种定量的、非形态的方法来研究太阳磁场在一系列空间尺度上的结构特性。分析的结果一方面将被用来对抗产生小尺度光球磁场的随机发电机模型，另一方面将与观测到的场分布相对抗。***

9309901 Lawrence Digital, photometric images of line-of-sight solar magnetic and velocity fields, obtained at high spatial resolution, will be analyzed using modern fractal, wavelet transform and percolation methods. This study will develop a quantitative, non- morphological, approach to the structural properties of solar magnetic fields over a range of spatial scales. The results of the analysis will be used to confront random dynamo models of the generation of small-scale photospheric magentic fields, on the one hand, with the observed field distributions, on the other. ***