  Strongly coupled plasmas in which the interaction energy exceeds the kinetic
energy play an important role in many astrophysical and laboratory systems
including compact stars, laser plasmas and dusty plasmas. They exhibit many
unusual collective properties, such as liquid or crystalline behaviour,
peculiar oscillation spectra and transport properties. Recently, strongly
coupled plasmas were studied in the presence of a strong magnetic field by
computer simulations, and strong modifications of their transport properties
and oscillation spectra were observed. While strong magnetization is common in
stellar systems it is practically impossible to achieve in complex plasmas due
to the large mass of the dust particles. Here we discuss a recently
demonstrated approach to achieve very strong "magnetization" by a rotation of
the neutral gas, and we present new results for macroscopic two-dimensional
systems.
