spatial scale, the existence of helical properties has been very commonly noticed with a broad range of techniques. First, the morphology of the coronal jets has been noted from X-ray and EUV images by various studies [e.g., @Shibata92; @Canfield96; @JiangY07; @ShenY12]. The frequency of helical structure in coronal jets is strongly dependent on the wavelength of observation. By looking only at X-ray images, @Shimojo96 reported a 10% occurrence of twisting within their observational sample. Using more recent Hinode/XRT observations, @Savcheva09b noted that 14% of their X-ray jets showed signs of twisting. In contrast, using EUV observations from the STEREO mission [@Kaiser08], @Nistico09 found that 31 out of 79 jet events presented a clear helical structure. From a sample of 54 jets observed in X-rays, @Moore13 found that 29 out of the 32 jets that also presented a cool component of emission at SDO/AIA 304 Å displayed a rotation about its axis in that channel. Helical structure and twisting motion are thus predominantly noted in the cooler EUV lines such as 304 Å. Using that particular bandwidth, several studies [e.g., @ShenY11; @ChenHD12; @HongJC13] have inferred the twisting rate and the helical morphology by analyzing the motion of well identified features within 