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Cited article:

The Magnetic Properties of Heating Events on High-temperature Active-region Loops

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The Astrophysical Journal 877 (2) 129 (2019)
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Modeling Coronal Response in Decaying Active Regions with Magnetic Flux Transport and Steady Heating

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The Astrophysical Journal 846 (2) 165 (2017)
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A new approach for modelling chromospheric evaporation in response to enhanced coronal heating

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Astronomy & Astrophysics 597 A81 (2017)
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DOPPLER SHIFT OF THE QUIET REGION MEASURED BY MERIDIONAL SCANS WITH THE EUV IMAGING SPECTROMETER ON BOARD HINODE

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The Astrophysical Journal 816 (1) 14 (2016)
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OBSERVATIONAL SIGNATURES OF CORONAL LOOP HEATING AND COOLING DRIVEN BY FOOTPOINT SHUFFLING

R. B. Dahlburg, G. Einaudi, B. D. Taylor, I. Ugarte-Urra, H. P. Warren, A. F. Rappazzo and M. Velli
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What can large-scale magnetohydrodynamic numerical experiments tell us about coronal heating?

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THE INFLUENCE OF NUMERICAL RESOLUTION ON CORONAL DENSITY IN HYDRODYNAMIC MODELS OF IMPULSIVE HEATING

S. J. Bradshaw and P. J. Cargill
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Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region

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Astronomy & Astrophysics 555 A123 (2013)
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ULTRAVIOLET SPECTROSCOPY OF RAPIDLY ROTATING SOLAR-MASS STARS: EMISSION-LINE REDSHIFTS AS A TEST OF THE SOLAR-STELLAR CONNECTION

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COMMISSION 10: SOLAR ACTIVITY

Lidia van Driel-Gesztelyi, Carolus J. Schrijver, James A. Klimchuk, et al.
Proceedings of the International Astronomical Union 7 (T28A) 69 (2011)
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