The Statistics of Polar Coronal Jets using XRT/Hinode

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Scientific paper

Recent observations of the polar coronal holes using the X-Ray Telescope on Hinode revealed how frequent x-ray jets occur. Previous observations were limited by cadence, spatial resolution and continuity. However, with XRT operations successfully underway, multiple weeks of polar observations can be used to provide improved statistics of some fundamental physical parameters of the jets. In particular, we will present results for the radial and transverse velocities, observed length and width, duration, and spatial distribution of some of the more than 200 jets XRT has observed to date. The observed changes in the structure of the region where the jets are formed seems to be well characterized by the Shibata-type reconnection model. Examples will be provided.

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