Interstellar turbulence I: observations and processes
BG Elmegreen, J Scalo - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract Turbulence affects the structure and motions of nearly all temperature and density
regimes in the interstellar gas. This two-part review summarizes the observations, theory …
regimes in the interstellar gas. This two-part review summarizes the observations, theory …
Astrophysical gyrokinetics: kinetic and fluid turbulent cascades in magnetized weakly collisional plasmas
This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …
astrophysical plasmas. It is motivated by observations of electromagnetic and density …
Heating of the solar chromosphere and corona by Alfvén wave turbulence
AA Van Ballegooijen, M Asgari-Targhi… - The Astrophysical …, 2011 - iopscience.iop.org
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 …
and dissipation of Alfvén waves in a coronal loop is developed. The model includes the …
Self-consistent coronal heating and solar wind acceleration from anisotropic magnetohydrodynamic turbulence
SR Cranmer, AA Van Ballegooijen… - The Astrophysical …, 2007 - iopscience.iop.org
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 …
rooted in solar coronal holes, streamers, and active regions. These models represent the …
On the generation, propagation, and reflection of Alfvén waves from the solar photosphere to the distant heliosphere
SR Cranmer, AA Van Ballegooijen - The Astrophysical Journal …, 2005 - iopscience.iop.org
We present a comprehensive model of the global properties of Alfvén waves in the solar
atmosphere and the fast solar wind. Linear non-WKB wave transport equations are solved …
atmosphere and the fast solar wind. Linear non-WKB wave transport equations are solved …
MHD turbulence: a biased review
AA Schekochihin - Journal of Plasma Physics, 2022 - cambridge.org
This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …
developments of the last few years in the context of the canonical time line (from Kolmogorov …
Coronal holes and the high-speed solar wind
SR Cranmer - Space Science Reviews, 2002 - Springer
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 …
and are associated with rapidly expanding magnetic fields and the acceleration of the high …
Evaluation of the turbulent energy cascade rates from the upper inertial range in the solar wind at 1 AU
BJ Vasquez, CW Smith, K Hamilton… - Journal of …, 2007 - Wiley Online Library
We construct a database from ACE spacecraft measurements of solar wind magnetic field
fluctuations at 1 AU which resolves∼ 2 decades in frequency at the high end of the inertial …
fluctuations at 1 AU which resolves∼ 2 decades in frequency at the high end of the inertial …
Wave turbulence in incompressible Hall magnetohydrodynamics
S Galtier - Journal of Plasma Physics, 2006 - cambridge.org
We investigate the steepening of the magnetic fluctuation power law spectra observed in the
inner Solar wind for frequencies higher than 0.5 Hz. This high frequency part of the spectrum …
inner Solar wind for frequencies higher than 0.5 Hz. This high frequency part of the spectrum …