A small-scale EUV jet in the quiet Sun region

Hong Junchao, hjcsolar@ynao.ac.cn, Yunnan Astronomical Observatory, China

Abstract
The commonly observed jets are the typical proxies of small-scale magnetic reconnection events in the solar atmosphere. We study a solar quiet-region jet observed by the Solar Dynamics Observatory and Ahead of Solar Terrestrial Relations Observatory. The correlation magnetograms and the calculated photospheric flows suggest that the jet is related to the interaction between the unipolar network and the emerged bipole driven by supergranular flows. By describing the EUV images on the quiet region, the jet actually follows the low non-potential magnetic loop and is injected into the nearby filament channel.