Yeah, plasmas pretty close but NOT a perfect conductor and the solar wind can have charge separation so....
So you'd be wrong on your assumptions
You really don't know what you are talking about, now, do you.
But I guess you also ask the plumber if he knows how to tighten the bolts and nuts, clock or anti-clockwise (and will probably give him the wrong direction as advise).
For those who want to know, every first year student of MHD and plasma physics is being taught is how the MHD approximation to plasma physics is done, and what the limitations are.
Also, the SW plasma is not a perfect conductor, but the conductivity is very very high, which means that the diffusion time of the magnetic field through the plasma is very very long, which means that
for appropriately chosen time intervals, e.g. the interaction of the SW with a comet, the field can be
assumed to be frozen in. And
really Hannes Alfvén already did that in his paper on cometary tails in 1957 (On the Theory of Cornet Tails, By H. ALFVEN. The Royal Institute of Technology, Stockholm, Tellus 9, 92 - 96, 1957)
I have explained this already several times, but Sol can just forget this again.
Also, with plasma physics being a very good theory, that does not mean that we have actually calculated everything already. As usual things are studied for situations that one encounters in experiments and or space missions. Never before was there a mission to a weakly outgassing comet in a weak magnetic field. Thus, any kind of wave generation in such a situation had not really been studied. However, pretty quickly after the surprise of finding such strong waves, the solution in plasma physics was found for the generation of these waves: a cross field current instability, which was already discussed in the literature, but never applied to a situation that had never been encountered.