Formation and Transport of Flux Transfer Events at Mercury

Computer Science

Scientific paper

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Scientific paper

We have developed a modified version of the Cooling model [3] to trace the motion of flux tubes generated by reconnection at Mercury, and in this paper we compare the model FTEs with observations of FTEs made by MESSENGER. We use these comparisons to determine the most likely location and orientation of the magnetic X-lines at Mercury's magnetopause during a variety of solar wind conditions.

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