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Cited article:

Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region

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Astronomy & Astrophysics 555 A123 (2013)
https://doi.org/10.1051/0004-6361/201321185

THE IMPORTANCE OF GEOMETRIC EFFECTS IN CORONAL LOOP MODELS

Zoran Mikić, Roberto Lionello, Yung Mok, Jon A. Linker and Amy R. Winebarger
The Astrophysical Journal 773 (2) 94 (2013)
https://doi.org/10.1088/0004-637X/773/2/94

PROTON, ELECTRON, AND ION HEATING IN THE FAST SOLAR WIND FROM NONLINEAR COUPLING BETWEEN ALFVÉNIC AND FAST-MODE TURBULENCE

Steven R. Cranmer and Adriaan A. van Ballegooijen
The Astrophysical Journal 754 (2) 92 (2012)
https://doi.org/10.1088/0004-637X/754/2/92

Turbulent coronal heating mechanisms: coupling of dynamics and thermodynamics

R. B. Dahlburg, G. Einaudi, A. F. Rappazzo and M. Velli
Astronomy & Astrophysics 544 L20 (2012)
https://doi.org/10.1051/0004-6361/201219752

Investigation of mass flows in the transition region and corona in a three-dimensional numerical model approach

P. Zacharias, H. Peter and S. Bingert
Astronomy & Astrophysics 531 A97 (2011)
https://doi.org/10.1051/0004-6361/201016047