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Tuesday 05 Sep 2017Exploring coronal mass ejection torque on solar rotation evolution

Matthew Gent - University of Exeter

4th Floor Interaction Area 11:05-11:20

It is known that stars rotate with an angular velocity and experience angular momentum loss throughout their evolution. Outflows such as stellar wind are an example of this and their impact on rotation evolution is believed to be well understood. My project was aimed at investigating the impact that coronal mass ejections have on main sequence solar mass stars.

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