Microjets in the line Hα in a polar coronal hole.

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Scientific paper

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Scientific paper

The properties of compact 3 - 4″small scale "isolated" jets of the chromospheric matter with velocities of 20 - 70 km/s, which were discovered on Hα limb filtergrams of an N-polar coronal hole, are described. A possible contribution of these events to mass and kinetic energy flows in the solar atmosphere is estimated. The nature of these microjets may be explained by combination of the effects of magnetic reconnection and diamagnetic pushing in divergent magnetic force lines.

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