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Cross-helicity dominated distributed chaos (CHDC) for magnetohydrodynamic(large-scale) and kinetic (small-scale) ranges of space plasmas has beenstudied using results of direct numerical simulations and of measurements madein the Earth's magnetosheath and in free solar wind by the instruments onboardof the Magnetospheric Multiscale Mission and CLUSTER spacecrafts. Existence oftwo generic types of transition from the magnetohydrodynamic (MHD) to kineticrange has been shown: 1) from the Kolmogorov-like (scaling) MHD turbulence tothe kinetic CHDC and 2) from the magnetohydrodynamic CHDC to the kinetic CHDC.Results of measurements in the magnetosheath of some other planets: Saturn(Cassini observations), Jupiter (Galileo observations), and Mercury (Messengerobservations), have been briefly discussed in this contest.

Cross-helicity and transition from magnetohydrodynamics to kinetics in space plasmas