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 …

Interplanetary (IP) shocks are fundamental building blocks of the heliosphere, and the
possibility to observe them in situ is crucial to address important aspects of energy …

Plasma flows with enhanced dynamic pressure, known as magnetosheath jets, are often
found downstream of collisionless shocks. As they propagate through the magnetosheath …

Abstract The Parker Solar Probe (PSP) and Solar Orbiter (SolO) missions opened a new
observational window in the inner heliosphere, which is finally accessible to direct …

In fast collisionless shocks, the density and magnetic field increase and the plasma is
heated. The compression and heating are ultimately determined by the Rankine–Hugoniot …

We analyze here an energetic proton enhancement in a sheath ahead of a slow
interplanetry coronal mass ejection (ICME) detected by Parker Solar Probe on June 30 …

How thermal particles are accelerated to suprathermal energies is an unsolved issue,
crucial for many astrophysical systems. We report novel observations of irregular, dispersive …

We review the current literature on the formation of coherent structures (CoSs) in strongly
turbulent 3D magnetized plasmas. CoSs [Current Sheets (CS), magnetic filaments, large …

We show here that highly polarized x-ray synchrotron radiation from young supernova
remnants (SNRs) can be modeled within the framework of diffusive shock acceleration …

Interplanetary shocks are fundamental constituents of the heliosphere, where they form as a
result of solar activity. We use previously unavailable measurements of interplanetary …