Danny McKenna - What is a model and how do we use them to understand Earth’s climate
1 NSTX-U/KSTAR 2013: Stability/rotation results for plasmas at/near n = 1 limit (S.A. Sabbagh, et al.)Oct. 21 st, 2013 High beta, MHD, and non-resonant.
High beta, MHD, and non-resonant magnetic braking by NTV in KSTAR
