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Cited article:

A Comprehensive Radiative Magnetohydrodynamics Simulation of Active Region Scale Flux Emergence from the Convection Zone to the Corona

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3D non-driven magnetic reconnection at multiple separators

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Magnetic Reconnections in the Presence of Three-Dimensional Magnetic Nulls and Quasi-Separatrix Layers

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Three-dimensional magnetic reconnection in astrophysical plasmas

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Determining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null points

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The Role of a Magnetic Topology Skeleton in a Solar Active Region

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The plasmoid instability in a confined solar flare

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A Cancellation Nanoflare Model for Solar Chromospheric and Coronal Heating

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The Astrophysical Journal Letters 862 (2) L24 (2018)
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Solar Magnetic Carpet III: Coronal Modelling of Synthetic Magnetograms

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THE STORAGE AND DISSIPATION OF MAGNETIC ENERGY IN THE QUIET SUN CORONA DETERMINED FROM SDO /HMI MAGNETOGRAMS

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Solar Magnetic Carpet II: Coronal Interactions of Small-Scale Magnetic Fields

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Review Article: MHD Wave Propagation Near Coronal Null Points of Magnetic Fields

J. A. McLaughlin, A. W. Hood and I. De Moortel
Space Science Reviews 158 (2-4) 205 (2011)
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ELLERMAN BOMBS AT HIGH RESOLUTION. I. MORPHOLOGICAL EVIDENCE FOR PHOTOSPHERIC RECONNECTION

Hiroko Watanabe, Gregal Vissers, Reizaburo Kitai, Luc Rouppe van der Voort and Robert J. Rutten
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NUMERICAL INVESTIGATION OF A CORONAL MASS EJECTION FROM AN ANEMONE ACTIVE REGION: RECONNECTION AND DEFLECTION OF THE 2005 AUGUST 22 ERUPTION

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

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The Astrophysical Journal 720 (1) 824 (2010)
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SOLAR CYCLE VARIATIONS OF CORONAL NULL POINTS: IMPLICATIONS FOR THE MAGNETIC BREAKOUT MODEL OF CORONAL MASS EJECTIONS

G. R. Cook, D. H. Mackay and Dibyendu Nandy
The Astrophysical Journal 704 (2) 1021 (2009)
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Recursive Reconnection and Magnetic Skeletons

C. E. Parnell, A. L. Haynes and K. Galsgaard
The Astrophysical Journal 675 (2) 1656 (2008)
https://doi.org/10.1086/527532

Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU?

Joseph E. Borovsky
Journal of Geophysical Research: Space Physics 113 (A8) (2008)
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Interaction of magnetic field systems leading to an X1.7 flare due to large-scale flux tube emergence

H. Li, B. Schmieder, M. T. Song and V. Bommier
Astronomy & Astrophysics 475 (3) 1081 (2007)
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Magnetohydrodynamic evolution of magnetic skeletons

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Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences 463 (2080) 1097 (2007)
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The Effect of the Relative Orientation between the Coronal Field and New Emerging Flux. I. Global Properties

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Structure and Dynamics of the Sun’s Open Magnetic Field

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The Astrophysical Journal 671 (1) 936 (2007)
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Flux tube disconnection: An example of three-dimensional reconnection

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Physics of Plasmas 14 (10) (2007)
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Astrophysics in 2005

Virginia Trimble, Markus J. Aschwanden and Carl J. Hansen
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Solar coronal heating by magnetic cancellation – II. Disconnected and unequal bipoles

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Monthly Notices of the Royal Astronomical Society 369 (1) 43 (2006)
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Dynamic Three‐dimensional Reconnection in a Separator Geometry with Two Null Points

D. I. Pontin and I. J. D. Craig
The Astrophysical Journal 642 (1) 568 (2006)
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Solar coronal heating by magnetic cancellation -- I. Connected equal bipoles

B. von Rekowski, C. E. Parnell and E. R. Priest
Monthly Notices of the Royal Astronomical Society 366 (1) 125 (2006)
https://doi.org/10.1111/j.1365-2966.2005.09801.x

The Three‐dimensional Interaction between Emerging Magnetic Flux and a Large‐Scale Coronal Field: Reconnection, Current Sheets, and Jets

V. Archontis, F. Moreno‐Insertis, K. Galsgaard and A. W. Hood
The Astrophysical Journal 635 (2) 1299 (2005)
https://doi.org/10.1086/497533

Coronal Heating at Separators and Separatrices

E. R. Priest, D. W. Longcope and J. Heyvaerts
The Astrophysical Journal 624 (2) 1057 (2005)
https://doi.org/10.1086/429312

Numerical Simulations of the Flux Tube Tectonics Model for Coronal Heating

C. Mellor, C. L. Gerrard, K. Galsgaard, A. W. Hood and E. R. Priest
Solar Physics 227 (1) 39 (2005)
https://doi.org/10.1007/s11207-005-1713-2