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.

中文翻译：

---

Jetlike CME 的原因和运动学

在本文中，我们根据太阳动力学天文台、太阳和日光层天文台以及太阳地球相关天文台的数据，对非典型太阳射流进行了多视点和多波长分析。通常认为日冕物质抛射（CME）是由低层大气中的大规模太阳爆发发展而来的。然而，2013 年 4 月 28 日喷流的运动学和空间演变指导我们，该喷流显然与宽度约为 25 度、速度为 450 公里/秒的狭窄 CME 相关。为了更好地理解喷流和 CME 之间的联系，我们从 AR 的视线磁力图进行了日冕势场外推。