What SDO tells us about structure and evolution of coronal bright points

Using magnetograms and coronal images from two instruments on board the Solar Dynamics Observatory (SDO), we study structure and evolution of a limited number of coronal bright points (CBPs). Our results show that the relation between CBPs and their magnetic footpoints is not simple. In some cases, CBP may appear as a bright portion of a larger loop (with clearly identifiable footpoints), and in some cases, an isolated CBP may develop between magnetic poles, which might not be the closest ones to each other or which might not be involved in the magnetic flux cancellation. We suggest that the magnetic connectivity responsible for formation of isolated coronal bright points is governed by the orientation of the large‐scale magnetic field. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

琼东沿岸泥质沉积常量元素地球化学特征

对南海北部陆架琼东沿岸泥质区$20孔进行了岩性、粒度和常量元素分析,初步探讨了该泥质区常量元素地球化学特征.S20孔岩性较均一,主要为黏土质粉砂,研究区受相对单一而稳定的水动力条件控制.常量元素含量变化符合“元素的粒度控制律”,R型因子分析结果表明,第一因子P2O5,MnO,TiO2,A12O3,Fe2O3和K2O等的...