In GitLab by @mkovari on May 19, 2020, 11:02
Jack Berkery et al of Columbia looked at 5000 experimental equilibria and produced a fit of the calculated no-wall beta limit against aspect ratio, internal inductance and pressure peaking. It is for NSTX so it should be relevant to ST reactors.

where

(The "poloidal magnetic field" has not been defined - see comments.)
https://iopscience.iop.org/article/10.1088/0029-5515/55/12/123007/pdf
The dependences in this fit are plotted here:Beta_limit.pdf
The key limits of applicability are
$A<1.8$,
$l_i>0.4$
Including the wall will make things more difficult as it depends on the geometry of the wall - especially how far it is from the plasma edge. This draft paper looks at this for MAST-U.
MAST-U_globalstability_v21.docx
The most conservative assumption is the no-wall limit. When a conducting wall is present the growth rate of unstable modes just above this limit is greatly reduced. Plasma rotation and kinetic effects can then make these modes stable, or they can be actively controlled. The use of ferromagnetic material such as Eurofer in the wall also has an effect. As all this is difficult to quantify, Chris Ham suggests we could go for the no-wall limit plus some percentage, e.g. no-wall limit times 1.2. We could make this a user input, resistive_wall_factor.
$\beta_{N,max}=f_{resistive-wall} \times \beta_{N,no-wall}$
This approach still requires sensible values for $l_i$ and $p_0/\langle p \rangle $, which is a matter for another day.
Any comments @stuartmuldrew, @schislet ?
Checklist
In GitLab by @mkovari on May 19, 2020, 11:02
Jack Berkery et al of Columbia looked at 5000 experimental equilibria and produced a fit of the calculated no-wall beta limit against aspect ratio, internal inductance and pressure peaking. It is for NSTX so it should be relevant to ST reactors.
where
(The "poloidal magnetic field" has not been defined - see comments.)
https://iopscience.iop.org/article/10.1088/0029-5515/55/12/123007/pdf
The dependences in this fit are plotted here:Beta_limit.pdf
The key limits of applicability are
$A<1.8$ ,
$l_i>0.4$
Including the wall will make things more difficult as it depends on the geometry of the wall - especially how far it is from the plasma edge. This draft paper looks at this for MAST-U.
MAST-U_globalstability_v21.docx
The most conservative assumption is the no-wall limit. When a conducting wall is present the growth rate of unstable modes just above this limit is greatly reduced. Plasma rotation and kinetic effects can then make these modes stable, or they can be actively controlled. The use of ferromagnetic material such as Eurofer in the wall also has an effect. As all this is difficult to quantify, Chris Ham suggests we could go for the no-wall limit plus some percentage, e.g. no-wall limit times 1.2. We could make this a user input,
$\beta_{N,max}=f_{resistive-wall} \times \beta_{N,no-wall}$
resistive_wall_factor.This approach still requires sensible values for$l_i$ and $p_0/\langle p \rangle $ , which is a matter for another day.
Any comments @stuartmuldrew, @schislet ?
Checklist