Abstract Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …

Abstract Solar Probe Plus (SPP) will be the first spacecraft to fly into the low solar corona.
SPP's main science goal is to determine the structure and dynamics of the Sun's coronal …

During the solar minimum, when the Sun is at its least active, the solar wind, is observed at
high latitudes as a predominantly fast (more than 500 kilometres per second), highly Alfvénic …

Abstract NASA's Solar Probe Plus (SPP) mission will make the first in situ measurements of
the solar corona and the birthplace of the solar wind. The FIELDS instrument suite on SPP …

Energy is required to heat the outer solar atmosphere to millions of degrees (refs,) and to
accelerate the solar wind to hundreds of kilometres per second (refs). Alfvén waves …

HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division
designed to explore the dynamic three-dimensional mechanisms controlling the physics of …

Shear-driven Transition to Isotropically Turbulent Solar Wind Outside the Alfvén Critical Zone -
IOPscience Skip to content IOP Science home Accessibility Help Search all IOPscience content …

This paper reviews Vlasov-based numerical methods used to model plasma in space
physics and astrophysics. Plasma consists of collectively behaving charged particles that …

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 …

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience Skip to
content IOP Science home Accessibility Help Search all IOPscience content Search Article …