An Alfvén wing is a stationary Alfvénic disturbance attached to a conducting obstacle moving through a magnetized plasma. In a super-Alfvénic flow its boundaries follow downstream characteristics.
For a stationary cold-plasma disturbance with obstaclespeed u0>uA, the characteristic slope is m=u02/uA2−1. It approaches u0/uA in the strongly super-Alfvénic limit.