Crossing the Earth's bow shock is known to crucially affect solar wind plasma including
changes in turbulent cascade. The present review summarizes results of more than 15 years …

Our understanding of processes occurring in the heliosphere historically began with
reduced dimensionality-one-dimensional (1D) and two-dimensional (2D) sketches and …

In many space, astrophysical, and laboratory plasmas the energy contained in the magnetic
field or plasma flow exceeds the thermal energy. Magnetic field (B) annihilation, often …

Studies of solar wind turbulence traditionally employ high-resolution magnetic field data, but
high-resolution measurements of ion and electron moments have been possible only …

Using observational data from the Magnetospheric Multiscale mission in the Earth's
magnetosheath, we estimate the energy cascade rate at three ranges of length scale …

The magnetosheath (MSH) plasma turbulence depends on the structure and properties of
the bow shock (BS). Under quasi-parallel (Q||) and quasi-perpendicular (Q⊥) BS …

Magnetospheric Multiscale (MMS) observations of plasma turbulence generated by a Kelvin–
Helmholtz (KH) event at the Earth's magnetopause are compared with a high-resolution two …

Decomposing the electric field (E) into the contributions from generalized Ohm's law
provides key insight into both nonlinear and dissipative dynamics across the full range of …

Composed of shocked solar wind, the Earth's magnetosheath serves as a natural laboratory
to study the transition of turbulence from low Alfvén Mach number, MA, to high M A. The …

The properties of turbulence observed within the plasma originating from the
magnetosheath and the magnetospheric boundary layer, which have been entrained within …