Add to ORKGThe heating of solar coronal loops by the resonant absorption or phase-mixing of incident wave energy is investigated in the framework of 3D nonlinear magnetohydrodynamics (MHD) by means of numerical simulations.status: publishe
Context. Recent numerical studies of oscillating flux tubes have established the significance of res...
Why the atmosphere of the Sun is orders of magnitudes hotter than its surface is a long-standing que...
Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves ...
The heating of magnetically closed structures (loops) in the solar corona by the resonant absorption...
Results are presented from magnetohydrodynamic (MHD) simulations of the phase-mixing and resonant ab...
The efficiency of resonant absorption of Alfvén waves as a solar coronal loop heating mechanism is s...
The heating of coronal loops by resonant absorption of Alfvén waves is studied in compressible, resi...
. We present the rst results of 2.5D nonlinear magnetohydrodynamic wave heating simulations of solar...
Context. The mechanism(s) behind coronal heating still elude(s) direct observation and modelling of ...
Results are presented from magnetohydrodynamic (MHD) simulations of the phase-mixing and resonant ab...
Results are presented from magnetohydrodynamic (MHD) simulations of the phase-mixing and resonant ab...
Context. The mechanism(s) behind coronal heating still elude(s) direct observation and modelling of ...
We present the first 2.5D numerical model calculations of the nonlinear wave dynamics and heating by...
We present the first 2.5 dimensional numerical model calculations of the nonlinear wave dynamics and...
© ESO, 2017. Context. Recent numerical studies of oscillating flux tubes have established the signif...
Context. Recent numerical studies of oscillating flux tubes have established the significance of res...
Why the atmosphere of the Sun is orders of magnitudes hotter than its surface is a long-standing que...
Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves ...
The heating of magnetically closed structures (loops) in the solar corona by the resonant absorption...
Results are presented from magnetohydrodynamic (MHD) simulations of the phase-mixing and resonant ab...
The efficiency of resonant absorption of Alfvén waves as a solar coronal loop heating mechanism is s...
The heating of coronal loops by resonant absorption of Alfvén waves is studied in compressible, resi...
. We present the rst results of 2.5D nonlinear magnetohydrodynamic wave heating simulations of solar...
Context. The mechanism(s) behind coronal heating still elude(s) direct observation and modelling of ...
Results are presented from magnetohydrodynamic (MHD) simulations of the phase-mixing and resonant ab...
Results are presented from magnetohydrodynamic (MHD) simulations of the phase-mixing and resonant ab...
Context. The mechanism(s) behind coronal heating still elude(s) direct observation and modelling of ...
We present the first 2.5D numerical model calculations of the nonlinear wave dynamics and heating by...
We present the first 2.5 dimensional numerical model calculations of the nonlinear wave dynamics and...
© ESO, 2017. Context. Recent numerical studies of oscillating flux tubes have established the signif...
Context. Recent numerical studies of oscillating flux tubes have established the significance of res...
Why the atmosphere of the Sun is orders of magnitudes hotter than its surface is a long-standing que...
Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves ...