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 …

Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …

Magnetic waves are a relevant component in the dynamics of the solar atmosphere. Their
significance has increased because of their potential as a remote diagnostic tool and their …

Plasma in the Sun's hot corona expands into the heliosphere as a supersonic and highly
magnetized solar wind. This paper provides an overview of our current understanding of …

Zank et al. developed a turbulence transport model for low-frequency incompressible
magnetohydrodynamic (MHD) turbulence in inhomogeneous flows in terms of the energy …

A detailed study of solar wind turbulence throughout the heliosphere in both the upwind and
downwind directions is presented. We use an incompressible magnetohydrodynamic (MHD) …

We present numerical simulations of reduced magnetohydrodynamic (RMHD) turbulence in
a magnetic flux tube at the center of a polar coronal hole. The model for the background …

The temperature dependence of the emission measure (EM) in the core of active regions
coronal loops is an important diagnostic of heating processes. Observations indicate that EM …

The solar transition region (TR) is the temperature regime from roughly 0.02 MK to 0.8 MK in
the solar atmosphere. It is the transition layer from the collisional and partially ionized …

Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …