In situ measurements of the solar wind and remote observations of coronal holes have
strongly implicated the resonant interaction with ion cyclotron waves as the responsible …

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 …

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 …

We solve the problem of propagation and dissipation of Alfvénic turbulence in a model solar
atmosphere consisting of a static photosphere and chromosphere, transition region, and …

We analyze measured proton and electron temperatures in the high-speed solar wind in
order to calculate the separate rates of heat deposition for protons and electrons. When …

By performing a one-dimensional magnetohydrodynamic simulation with radiative cooling
and thermal conduction, we show that the coronal heating and the fast solar wind …

Numerous problems in space physics and astrophysics require a detailed understanding of
the transport and dissipation of low-frequency turbulence in an expanding magnetized flow …

II. Transport of Nearly Incompressible Magnetohydrodynamic Turbulence from 1 to 75 au -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

Abstract The Parker Solar Probe (PSP) achieved its first orbit perihelion on 2018 November
6, reaching a heliocentric distance of about 0.165 au (35.55 R⊙). Here, we study the …

The heating of the lower solar corona is examined using numerical simulations and
theoretical models of magnetohydrodynamic turbulence in open magnetic regions. A …