HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division
designed to explore the dynamic three-dimensional mechanisms controlling the physics of …

The complex interaction between shocks and plasma turbulence is extremely important to
address crucial features of energy conversion in a broad range of astrophysical systems. We …

A novel multispacecraft technique applied to Magnetospheric Multiscale Mission data in the
Earth's magnetosheath enables evaluation of the energy cascade rate from the full Yaglom's …

Plasma turbulence involves complex, nonlinear interactions of electromagnetic fields and
charged particles across multiple scales. Studying these phenomena in space plasmas, like …

We have studied the decay of turbulence in the solar wind. Fluctuations carried by the
expanding wind are naturally damped because of flux conservation, slowing down the …

We present evidence for nonlocal contributions to the turbulent energy cascade in
magnetohydrodynamic (MHD) plasmas. Therefore, we revisit a well-known result derived …

Measuring the energy cascade rate in space plasmas is a challenging task for several
reasons. This quantity is (i) inherently three-dimensional (ii) scale-dependent,(iii) anisotropic …

The geomagnetic storm that occurred on April 23-24, 2023 was the largest such event in
nearly the last two decades. As the solar cycle begins to increase towards the maximum …

The energy dissipation in collisionless plasmas as the solar wind is not yet fully understood.
The intermittent nature of magnetic structures appears to be a fundamental part of the …

We present evidence for nonlocal contributions to the turbulent energy cascade in
magnetohydrodynamic (MHD) plasmas. Therefore, we revisit a well-known result derived …