A model for the formation of the active region corona driven by magnetic flux emergence
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Title
A model for the formation of the active region corona driven by magnetic flux emergence
Authors
Keywords
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Journal
ASTRONOMY & ASTROPHYSICS
Volume 564, Issue -, Pages A12
Publisher
EDP Sciences
Online
2014-02-25
DOI
10.1051/0004-6361/201322859
References
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Related references
Note: Only part of the references are listed.- Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region
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- ON THE ANISOTROPY IN EXPANSION OF MAGNETIC FLUX TUBES IN THE SOLAR CORONA
- (2013) A. Malanushenko et al. ASTROPHYSICAL JOURNAL
- THERMAL NON-EQUILIBRIUM REVISITED: A HEATING MODEL FOR CORONAL LOOPS
- (2013) Roberto Lionello et al. ASTROPHYSICAL JOURNAL
- Constant cross section of loops in the solar corona
- (2012) H. Peter et al. ASTRONOMY & ASTROPHYSICS
- Nanoflare statistics in an active region 3D MHD coronal model
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- A METHOD FOR DATA-DRIVEN SIMULATIONS OF EVOLVING SOLAR ACTIVE REGIONS
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- Intermittent heating in the solar corona employing a 3D MHD model
- (2011) S. Bingert et al. ASTRONOMY & ASTROPHYSICS
- HEATING OF THE SOLAR CHROMOSPHERE AND CORONA BY ALFVÉN WAVE TURBULENCE
- (2011) A. A. van Ballegooijen et al. ASTROPHYSICAL JOURNAL
- Initial Calibration of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)
- (2011) Paul Boerner et al. SOLAR PHYSICS
- ON REDSHIFTS AND BLUESHIFTS IN THE TRANSITION REGION AND CORONA
- (2010) V. H. Hansteen et al. ASTROPHYSICAL JOURNAL
- SIMULATION OF THE FORMATION OF A SOLAR ACTIVE REGION
- (2010) M. C. M. Cheung et al. ASTROPHYSICAL JOURNAL
- TWISTED FLUX TUBE EMERGENCE FROM THE CONVECTION ZONE TO THE CORONA. II. LATER STATES
- (2009) Juan Martínez-Sykora et al. ASTROPHYSICAL JOURNAL
- Penumbral Structure and Outflows in Simulated Sunspots
- (2009) M. Rempel et al. SCIENCE
- Twisted Flux Tube Emergence From the Convection Zone to the Corona
- (2008) Juan Martínez‐Sykora et al. ASTROPHYSICAL JOURNAL
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