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Cited article:

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A Comprehensive Simulation of Solar Wind Formation from the Solar Interior: Significant Cross-field Energy Transport by Interchange Reconnection near the Sun

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A New Broadening Technique of the Numerically Unresolved Solar Transition Region and Its Effect on the Spectroscopic Synthesis Using Coronal Approximation

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Resonances in a Coronal Loop Driven by Torsional Alfvén Waves Propagating from the Photosphere

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Weak Damping of Propagating MHD Kink Waves in the Quiescent Corona

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Fast Solar Wind Driven by Parametric Decay Instability and Alfvén Wave Turbulence

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Turbulence in a Coronal Loop Excited by Photospheric Motions

Giuseppina Nigro, Francesco Malara, Antonio Vecchio, Leonardo Primavera, Francesca Di Mare, Vincenzo Carbone and Pierluigi Veltri
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Electron Heating by Kinetic Alfvén Waves in Coronal Loop Turbulence

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A Self-consistent Model of the Coronal Heating and Solar Wind Acceleration Including Compressible and Incompressible Heating Processes

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Frequency-dependent Alfvén-wave Propagation in the Solar Wind: Onset and Suppression of Parametric Decay Instability

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Monthly Notices of the Royal Astronomical Society 463 (1) 502 (2016)
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CLOSED-FIELD CORONAL HEATING DRIVEN BY WAVE TURBULENCE

Cooper Downs, Roberto Lionello, Zoran Mikić, Jon A Linker and Marco Velli
The Astrophysical Journal 832 (2) 180 (2016)
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CONNECTING THE SUN'S HIGH-RESOLUTION MAGNETIC CARPET TO THE TURBULENT HELIOSPHERE

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Saturation of StellarWinds from Young Suns

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ON THE ORIGIN OF THE 1/ f SPECTRUM IN THE SOLAR WIND MAGNETIC FIELD

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NON-THERMAL RESPONSE OF THE CORONA TO THE MAGNETIC FLUX DISPERSAL IN THE PHOTOSPHERE OF A DECAYING ACTIVE REGION

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