Abstract
We present an analysis of high cadence observations of solar jets observed in the Extreme Ultraviolet (EUV), at 304 A, with the Atmospheric Imaging Assembly instrument aboard the Solar Dynamics Observatory (SDO). The jets in our sample lie very close to the solar limb to minimize projection effects. Two of the events show clear helical patterns during ejection. We also find that some of the jets are recurrent and that most of them cannot overcome solar gravity.
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