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The ubiquitous solar jets or jet-like activities are generally regarded as animportant source of energy and mass input to the upper solar atmosphere and thesolar wind. However, questions about their triggering and driving mechanismsare not completely understood. By taking advantage of high temporal and highspatial resolution stereoscopic observations taken by the Solar DynamicObservatory (SDO) and the Solar Terrestrial Relations Observatory (STEREO), wereport an intriguing two-sided-loop jet occurred on 2013 June 02, which wasdynamically associated with the eruption of a mini-filament below an overlyinglarge filament, and two distinct reconnection processes are identified duringthe formation stage. The SDO observations reveals that the two-sided-loop jetshowed a concave shape with a projection speed of about 80 - 136. From theother view angle, the STEREO ahead observations clearly showed that thetrajectory of the two arms of the two-sided-loop were along the cavity magneticfield lines hosting the large filament. Contrary to the well-acceptedtheoretical model, the present observation sheds new light on our understandingof the formation mechanism of two-sided-loop jets. Moreover, the eruption ofthe two-sided-loop jet not only supplied mass to the overlying large filament,but also provided a rare opportunity to diagnose the magnetic structure of theoverlying large filament via the method of three-dimensional reconstruction.

Stereoscopic Observations of an Erupting Mini-filament Driven Two-Sided-Loop Jet and the Applications for Diagnosing Filament Magnetic field