论文标题
类似喷射的CME的原因和运动学
Cause and Kinematics of a Jet-Like CME
论文作者
论文摘要
在本文中，我们介绍了基于太阳能动力学观测站，太阳能和地球层观测站和太阳陆地关系天文台的数据，介绍了非典型太阳喷气机的多波长和多波长分析。通常认为，冠状质量弹出（CME）是由下部大气中的大型太阳喷发发展而成的。然而，2013年4月28日，射流的运动学和空间演化指导我们显然与狭窄的CME相关，其宽度约为25度，速度为450 km/s。为了更好地理解射流与CME之间的联系，我们从AR的视线磁图进行了冠状电势场外推。推断出来的是，喷气喷发遵循来自源区域的开放磁场线完全相同的路径，该路径为射流材料从太阳能表面逃到外电晕提供了途径。
In this article, we present the multi-viewpoint and multi-wavelength analysis of an atypical solar jet based on the data from Solar Dynamics Observatory, SOlar, and Heliospheric Observatory, and Solar TErrestrial RElations Observatory. It is usually believed that the coronal mass ejections (CMEs) are developed from the large scale solar eruptions in the lower atmosphere. However, the kinematical and spatial evolution of the jet on 2013 April 28 guide us that the jet was clearly associated with a narrow CME having a width of approx 25 degrees with a speed of 450 km/s. To better understand the link between the jet and the CME, we did the coronal potential field extrapolation from the line of sight magnetogram of the AR. The extrapolations present that the jet eruption follows exactly the same path of the open magnetic field lines from the source region which provides the route for the jet material to escape from the solar surface towards the outer corona.
