When discussing research in physics and in science more generally, it is common to ascribe
equal importance to the three components of the scientific trinity: theoretical, experimental …

The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

The fast solar wind's high speeds and non-thermal features require that considerable
heating occurs well above the Sun's surface. Two leading theories seem incompatible: low …

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 …

A comprehensive overview is presented of recent observational and theoretical results on
solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence …

This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

The magnetic field experiment on ACE provides continuous measurements of the local
magnetic field in the interplanetary medium. These measurements are essential in the …

The dissipation range for interplanetary magnetic field fluctuations is formed by those
fluctuations with spatial scales comparable to the gyroradius or ion inertial length of a …

We show the first three dimensional (3D) dispersion relations and k spectra of magnetic
turbulence in the solar wind at subproton scales. We used the Cluster data with short …

We report the first direct determination of the dissipation range of magnetofluid turbulence in
the solar wind at the electron scales. Combining high resolution magnetic and electric field …