▪ Abstract Turbulence affects the structure and motions of nearly all temperature and density
regimes in the interstellar gas. This two-part review summarizes the observations, theory …

In this article, we state and review the premises on which a successful asymptotic closure of
the moment equations of wave turbulence is based, describe how and why this closure …

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

ABSTRACT A three-dimensional magnetohydrodynamic (MHD) model for the propagation
and dissipation of Alfvén waves in a coronal loop is developed. The model includes the …

We present a series of models for the plasma properties along open magnetic flux tubes
rooted in solar coronal holes, streamers, and active regions. These models represent the …

We present a comprehensive model of the global properties of Alfvén waves in the solar
atmosphere and the fast solar wind. Linear non-WKB wave transport equations are solved …

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

Coronal holes are the lowest density plasma components of the Sun's outer atmosphere,
and are associated with rapidly expanding magnetic fields and the acceleration of the high …

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 investigate the steepening of the magnetic fluctuation power law spectra observed in the
inner Solar wind for frequencies higher than 0.5 Hz. This high frequency part of the spectrum …