Counterrotation in magnetocentrifugally driven jets and other winds
C. Sauty, V. Cayatte, J. J. G. Lima, T. Matsakos, K. Tsinganos

TL;DR
This paper demonstrates that counterrotation in magnetocentrifugally driven jets and winds can naturally occur within ideal MHD theory, without contradicting the jet launching mechanism, and can be transient or layer-specific.
Contribution
It shows that counterrotation in jets and winds is compatible with magnetocentrifugal acceleration and can arise from flow deceleration, expanding understanding of jet dynamics.
Findings
Counterrotation can occur naturally in ideal MHD flows.
Flow deceleration below a threshold causes rotation direction change.
Counterrotation may be temporary and layer-specific.
Abstract
Rotation measurement in jets from T Tauri stars is a rather difficult task. Some jets seem to be rotating in a direction opposite to that of the underlying disk, although it is not yet clear if this affects the totality or part of the outflows. On the other hand, Ulysses data also suggest that the solar wind may rotate in two opposite ways between the northern and southern hemispheres. We show that this result is not as surprising as it may seem and that it emerges naturally from the ideal MHD equations. Specifically, counterrotating jets neither contradict the magnetocentrifugal driving of the flow nor prevent extraction of angular momentum from the disk. The demonstration of this result is shown by combining the ideal MHD equations for steady axisymmetric flows. Provided that the jet is decelerated below some given threshold beyond the Alfven surface, the flow will change its…
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