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 …

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 …

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 …

A primary goal of the Parker Solar Probe (PSP) Mission is to answer the outstanding
question of how the solar corona plasma is heated to the high temperatures needed for the …

Shell models of hydrodynamic turbulence originated in the seventies. Their main aim was to
describe the statistics of homogeneous and isotropic turbulence in spectral space, using a …

Self-similarity may originate from two origins: ie, the process memory and the process'
increments “infinite” variance. A distinction is attempted by employing the natural time χ …

A number of theoretical and observational considerations suggest that coronal loops are
bundles of unresolved, impulsively heated strands. This" nanoflare" model, as it is …

Collisionless Plasmas in Astrophysics examines the unique properties of media without
collisions in plasma physics. Experts in this field, the authors present the first book to …

The small-scale dynamo plays a substantial role in magnetizing the Universe under a large
range of conditions, including subsonic turbulence at low Mach numbers, highly supersonic …

The objective of this review article is to critically analyze turbulence and its role in the solar
atmosphere and solar wind, as well as to provide a tutorial overview of topics worth …