In theory, the difference between the slopes of the N II and H alpha structure functions will allow us to estimate the term $\delta\kappa$ from Brunt & Mac Low (2004).
I already have this for [N II] from Arthur et al.
It would be good to get it for 30 Dor also. The problem with the current results is that there is a degeneracy with the seeing width for both lines. Therefore, it is important to use the same s0 for both.
So @JavGVastro could you please run another analysis like ci-MUSE-Dor-N.ipynb but with the seeing width fixed at the value found for Ha
In theory, the difference between the slopes of the N II and H alpha structure functions will allow us to estimate the term $\delta\kappa$ from Brunt & Mac Low (2004).
I already have this for [N II] from Arthur et al.
It would be good to get it for 30 Dor also. The problem with the current results is that there is a degeneracy with the seeing width for both lines. Therefore, it is important to use the same s0 for both.
So @JavGVastro could you please run another analysis like ci-MUSE-Dor-N.ipynb but with the seeing width fixed at the value found for Ha
H alpha
[N II]