“…The induced local plasma current, J and magnetic flux density, B, produces a strong J × B Lorentz force which accelerates a highly energetic plasma to stagnate on axis in about 100 ns. This stagnation and subsequent magnetic energy conversion produces an intense 10 ns X-ray radiation pulse [43,53]. The intense X-ray pulse can then be used for radiation-material interaction studies [44,42,45], environments for indirect drive inertial confinement fusion (ICF) applications [42,45,43], or for pursuing laboratory-based astrophysics environments [45,51,54,15,9,22].…”