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Fig. 1

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Top panels: SDO/AIA images of the polar coronal hole jet. The wavelength corresponding to each channel is given in the panels. The rectangular box in each frame marks the location of the pixels used to generate the light curves in Fig. 4. Bottom panels: STEREO/SECCHI EUVI images of the same jet. The position of the jet is not obvious in the 195 Å bandpass but can be seen clearly above the limb in 304 Å.

This figure is made of several images, please see below:

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