Spatially resolved solar spectra

Solar surface magneto-convection appears as granulation pattern that impacts spectral lines in terms of both shape and wavelength. Such induced effects also tend to vary over...太阳表面的磁对流呈现为米粒组织结构，该结构会在形状与波长两个维度对光谱线产生影响。此类感应效应亦往往随……发生变化。