恒星磁场

本文最后还对红外CCD、紫外CCD、弱光CCD在太阳磁场测量和太阳恒星磁场观测的应用进行了介绍。

In the end , the applications of infrared CCD , ultraviolet CCD and weak-light CCD in the observation of sun magnetic field and sun stellar magnetic field are introduced .

本文综述了与恒星磁场测量有关的、太阳磁场若干观测特征。

In this paper , we have reviewed the observational characteristics of solar magnetic fields in these aspects which are relevant to stellar magnetic field measurements .

恒星形成区磁场的VLBI测量

VLBI measurements of magnetic field strength in a region of star formation

科研小组推断认为，这个推动因素来自于包括太阳系在内的银河系内众多恒星系统之间的磁场作用。

The scientific group infers believed that this impetus factor from including in solar system 's Milky Way between the numerous stellar system 's magnetic field function .

天文学家们利用一对不同寻常的附近恒星，首次拍下了一颗恒星磁场的图像，该磁场并非太阳产生的。

Taking advantage of an unusual pair of nearby stars , astronomers have for the first time captured images of a magnetic field generated by a star other than our sun .