Mode decoupling during retrorefraction as an explanation for bizarre radar echoes from icy moons

The two concepts of mode decoupling and retrorefraction are combined to explain the strength, distribution, and other features of the radar echoes from Europa, Ganymede, and Callisto. A decoupling of two characteristic modes of propagation appears to be a key to an understanding of the anomalous distribution of power among the polarized components of the echoes. Causes of the decoupling are proposed and their morphological implications are introduced.