A detailed study of solar wind turbulence throughout the heliosphere in both the upwind and
downwind directions is presented. We use an incompressible magnetohydrodynamic (MHD) …

The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed
largely in the early 1990s, together with an important extension to inhomogeneous flows in …

Abstract In October 2017, the Scientific Committee on Solar-Terrestrial Physics (SCOSTEP)
Bureau established a committee for the design of SCOSTEP's Next Scientific Programme …

Shock waves, as shown by simulations and observations, can generate high levels of
downstream vortical turbulence, including magnetic islands. We consider a combination of …

In this paper we investigate spectral and phase coherence properties of magnetic
fluctuations in the vicinity of the spectral transition from large, magnetohydrodynamic to sub …

Small-amplitude fluctuations in the magnetized solar wind are measured typically by a
single spacecraft. In the magnetohydrodynamics (MHD) description, fluctuations are typically …

We explore the role of heliospheric magnetic field configurations and conditions that favor
the generation and confinement of small-scale magnetic islands associated with atypical …

Context. Aims. We systematically search for magnetic flux rope structures in the solar wind to
within the closest distance to the Sun of~ 0.13 AU, using data from the third and fourth orbits …

We report observations of reconnection exhausts in the Heliospheric Current Sheet (HCS)
during Parker Solar Probe Encounters 08 and 07, at 16 Rs and 20 Rs, respectively …

Magnetic reconnection is a primary driver of particle acceleration processes in space and
astrophysical plasmas. Understanding how particles are accelerated and the resulting …