Abstract The Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Solar
Probe Plus is a four sensor instrument suite that provides complete measurements of the …

Coronal holes are the darkest and least active regions of the Sun, as observed both on the
solar disk and above the solar limb. Coronal holes are associated with rapidly expanding …

We present a new version of the Alfvén wave solar model, a global model from the upper
chromosphere to the corona and the heliosphere. The coronal heating and solar wind …

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 …

The basic mechanisms responsible for producing winds from cool, late-type stars are still
largely unknown. We take inspiration from recent progress in understanding solar wind …

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 …

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …

We consider ion heating by turbulent Alfvén waves (AWs) and kinetic Alfvén waves (KAWs)
with wavelengths (measured perpendicular to the magnetic field) that are comparable to the …

This paper studies the turbulent cascade of magnetic energy in weakly collisional
magnetized plasmas. A cascade model is presented, based on the assumptions of local …