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Home All issues A&A, 490 1 (2008) 353-356 Article references

Articles citing this article

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Cited article:

Simulating the Photospheric to Coronal Plasma Using Magnetohydrodyanamic Characteristics. II. Reflections on Non-reflecting Boundary Conditions

N. Dylan Kee, Lucas A. Tarr, Peter W. Schuck, Mark G. Linton and James E. Leake
The Astrophysical Journal 983 (1) 80 (2025)
https://doi.org/10.3847/1538-4357/adb132

Effect of Magnetic Diffusion in the Chromosphere on the Solar Wind

Masato Matsuoka, Takeru K. Suzuki, Takato Tokuno and Kensuke Kakiuchi
The Astrophysical Journal 970 (1) 16 (2024)
https://doi.org/10.3847/1538-4357/ad496b

Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions

Lucas A. Tarr, N. Dylan Kee, Mark G. Linton, Peter W. Schuck and James E. Leake
The Astrophysical Journal Supplement Series 270 (2) 30 (2024)
https://doi.org/10.3847/1538-4365/ad0e0c

Flare Reconnection-driven Magnetic Field and Lorentz Force Variations at the Sun’s Surface

Krzysztof Barczynski, Guillaume Aulanier, Sophie Masson and Michael S. Wheatland
The Astrophysical Journal 877 (2) 67 (2019)
https://doi.org/10.3847/1538-4357/ab1b3d

Three dimensional magnetohydrodynamic simulation of linearly polarised Alfven wave dynamics in Arnold-Beltrami-Childress magnetic field

D. Tsiklauri
Physics of Plasmas 21 (5) (2014)
https://doi.org/10.1063/1.4875920

SIGMOIDAL ACTIVE REGION ON THE SUN: COMPARISON OF A MAGNETOHYDRODYNAMICAL SIMULATION AND A NONLINEAR FORCE-FREE FIELD MODEL

A. Savcheva, E. Pariat, A. van Ballegooijen, G. Aulanier and E. DeLuca
The Astrophysical Journal 750 (1) 15 (2012)
https://doi.org/10.1088/0004-637X/750/1/15

CONNECTING THE SUN AND THE SOLAR WIND: THE FIRST 2.5-DIMENSIONAL SELF-CONSISTENT MHD SIMULATION UNDER THE ALFVÉN WAVE SCENARIO

Takuma Matsumoto and Takeru Ken Suzuki
The Astrophysical Journal 749 (1) 8 (2012)
https://doi.org/10.1088/0004-637X/749/1/8

COUPLING THE SOLAR DYNAMO AND THE CORONA: WIND PROPERTIES, MASS, AND MOMENTUM LOSSES DURING AN ACTIVITY CYCLE

Rui F. Pinto, Allan Sacha Brun, Laurène Jouve and Roland Grappin
The Astrophysical Journal 737 (2) 72 (2011)
https://doi.org/10.1088/0004-637X/737/2/72

CAN THE SOLAR WIND BE DRIVEN BY MAGNETIC RECONNECTION IN THE SUN'S MAGNETIC CARPET?

Steven R. Cranmer and Adriaan A. van Ballegooijen
The Astrophysical Journal 720 (1) 824 (2010)
https://doi.org/10.1088/0004-637X/720/1/824

3D MHD modelling of a chromosphere above the sun's convective zone

Rui Pinto and Sacha Brun
Proceedings of the International Astronomical Union 6 (S271) 393 (2010)
https://doi.org/10.1017/S1743921311017959

FORMATION OF TORUS-UNSTABLE FLUX ROPES AND ELECTRIC CURRENTS IN ERUPTING SIGMOIDS

G. Aulanier, T. Török, P. Démoulin and E. E. DeLuca
The Astrophysical Journal 708 (1) 314 (2010)
https://doi.org/10.1088/0004-637X/708/1/314

ELECTRON TRANSPORT IN CORONAL LOOPS: THE INFLUENCE OF THE EXPONENTIAL SEPARATION OF MAGNETIC FIELD LINES

R. Bitane, G. Zimbardo and P. Veltri
The Astrophysical Journal 719 (2) 1912 (2010)
https://doi.org/10.1088/0004-637X/719/2/1912

Coronal heating by magnetic reconnection in loops with zero net current

A. W. Hood, P. K. Browning and R. A. M. Van der Linden
Astronomy & Astrophysics 506 (2) 913 (2009)
https://doi.org/10.1051/0004-6361/200912285