Cohen, O.; Yadav, R.; Garraffo, Cecilia; Saar, S. H.; Wolk, S. J.; Kashyap, V. L.; Drake, Jeremy J.; Pillitteri, Ignazio
(2017)
Observations indicate that magnetic fields in rapidly rotating stars are very strong, on both small and large scales. What is the nature of the resulting corona? Here we seek to shed some light on this question. We use the ...