I'm not sure which of the several Stenzel and Gekelman papers I linked that you are referring to, but I don't see "wrong way" current flow in any of them that is unexplained in the papers as being atypical of reconnection observations.
And yes, MHD is a bunch of crap when it comes to modeling dynamic plasma systems.
Let us quote Alfven on MHD theory:
Then maybe you should look up
post 105 where I comment on the
last paper that you quote in post 102. Read my post 105 again and read my explanation about DLs above again, then think once more about what you write (quoted above).
Just to be clear:
In Fig. 2 of said paper you see the X-Z plane of the experiment which is perpendicular to the axis of the plasma device. It shows the magnetic field topology and the plasma flow, both typical for reconnection.
The current sheet is in the middle at Z=0, going into (or out of) the plane of the figure. The current is flowing in the Y direction.
Gekelman increases the voltage over the machine, driving stronger current in the Y direction, thus creating double layers which will accelerate particles in the Y direction (that is perpendicular to the direction in which reconnection accelerates particles, which is in the X direction in the experiment). Therefore, these double layers, artificially created after reconnection is already taking place, cannot and will not accelerate the particles in the reconnection exhausts.
It is really very simple, you just have to keep the coordinate system in mind, and then it is self explanatory.
MHD is a wonderful tool, for those who know how to use it, which would be any plasma(astro)physicist these days. The comments by Alfvén stem from a time when MHD was used as a tool without thinking about the how and what. Frozen in condition was assumed to be true, and that was that.
Nowadays we get taught that that cannot be. No plasma is infinitely conducting, and thus there is a so called diffusion time of the plasma. The better the conductivity, the longer the time. Then for processes that are shorter than the diffusion time, the frozen in condition can be assumed valid, for processes that take longer the frozen in condition cannot be used.
MDH is an averaged plasma physcis theory, over the longest time and length scales of the plasma. So, whenever you are modeling stuff that is on scales much larger than the greatest gyroradius and on time scales longer than the longest gyroperiod, MDH is valid. If you want to look at smaller scale processes, then you have to revert to plasma physics.
Again, it is all very simple.
In the Earth's magnetosphere, for example, many a process can be described with MHD and even with the frozen in condition, but other processes not.
Here my good friend Tony Lui discusses regions in the Earth's magnetotail where the frozen in condition breaks down.