Parker solar probe: Four years of discoveries at solar cycle minimum
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 …
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
Scaling laws for the energy transfer in space plasma turbulence
R Marino, L Sorriso-Valvo - Physics Reports, 2023 - Elsevier
One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
Theory and transport of nearly incompressible magnetohydrodynamic turbulence
GP Zank, L Adhikari, P Hunana, D Shiota… - The Astrophysical …, 2017 - iopscience.iop.org
The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed
largely in the early 1990s, together with an important extension to inhomogeneous flows in …
largely in the early 1990s, together with an important extension to inhomogeneous flows in …
The evolution and role of solar wind turbulence in the inner heliosphere
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 …
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
Intermittency, nonlinear dynamics and dissipation in the solar wind and astrophysical plasmas
An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …
Coronal heating by magnetohydrodynamic turbulence driven by reflected low-frequency waves
WH Matthaeus, GP Zank, S Oughton… - The Astrophysical …, 1999 - iopscience.iop.org
ABSTRACT A candidate mechanism for the heating of the solar corona in open field line
regions is described. The interaction of Alfvén waves, generated in the photosphere or …
regions is described. The interaction of Alfvén waves, generated in the photosphere or …
Turbulence transport in the solar corona: Theory, modeling, and Parker Solar Probe
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 …
question of how the solar corona plasma is heated to the high temperatures needed for the …
Generation of the fast solar wind: A review with emphasis on the resonant cyclotron interaction
JV Hollweg, PA Isenberg - Journal of Geophysical Research …, 2002 - Wiley Online Library
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 …
strongly implicated the resonant interaction with ion cyclotron waves as the responsible …
Turbulence in space plasmas: Who needs it?
WH Matthaeus - Physics of Plasmas, 2021 - pubs.aip.org
The complex nonlinear dynamical phenomenon described as turbulence, is known to have
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …
a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper …
The solar magnetic field
SK Solanki, B Inhester… - Reports on progress in …, 2006 - iopscience.iop.org
The magnetic field of the Sun is the underlying cause of the many diverse phenomena
combined under the heading of solar activity. Here we describe the magnetic field as it …
combined under the heading of solar activity. Here we describe the magnetic field as it …