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Shuhong Yang et al 2016 ApJL 833 L18

Observations from the Interface Region Imaging Spectrograph show how a light wall on the solar surface responds when flare material hits its base: the wall brightens at the base and then increases in height.

C. Garraffo et al 2016 ApJL 833 L4

3D MHD modeling of Proxima Centauri’s wind and magnetic field suggest that Proxima Centauri b is subject to stellar wind pressures of more than 2000 times those experienced by Earth from the solar wind.

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