Energetic particles are accelerated in rich profusion at sites throughout the heliosphere.
They come from solar flares in the low corona, from shock waves driven outward by coronal …

In this review we will focus on a topic of fundamental importance for both astrophysics and
plasma physics, namely the occurrence of large-amplitude low-frequency fluctuations of the …

Mechanisms for the deposition of heat in the lower coronal plasma are discussed,
emphasizing recent attempts to reconcile the fluid and kinetic perspectives. Structures at …

Using 5 years of spacecraft data from near Earth orbit, we investigate the correlation
anisotropy of solar wind magnetohydrodynamic-scale fluctuations and show that the nature …

We construct a database from ACE spacecraft measurements of solar wind magnetic field
fluctuations at 1 AU which resolves∼ 2 decades in frequency at the high end of the inertial …

We perform a test of MHD turbulent cascade theory in the solar wind and directly evaluate
the contribution of local turbulence to heating the solar wind at 1 AU. We look at turbulent …

Solar wind magnetic fluctuation power spectra at frequencies ƒ< 1 Hz are commonly
observed to have the approximate power law dependence ƒ− 5/3. These observations may …

The turbulent flows and tangled magnetic fields of the Earth's plasma sheet are explored
theoretically and by means of ISEE‐2 plasma and magnetic‐field measurements. The goal …

We study anisotropic magnetohydrodynamic (MHD) turbulence in the slow solar wind
measured by Parker Solar Probe (PSP) and Solar Orbiter (SolO) during its first orbit from the …

We examine the convergence of third-order structure function expressions derived to
measure the rate of turbulent energy cascade within the solar wind using Advanced …