D. H. Mackay

THE INFLUENCE OF THE MAGNETIC FIELD ON RUNNING PENUMBRAL WAVES IN THE SOLAR CHROMOSPHERE

T. Doorsselaere, D. Mackay, P. Keys, 2013, 1310.7939.

SOLAR CYCLE VARIATIONS OF CORONAL NULL POINTS: IMPLICATIONS FOR THE MAGNETIC BREAKOUT MODEL OF CORONAL MASS EJECTIONS

G. R. Cook, D. Nandy, D. Mackay, 2009 .

Inferring X-ray coronal structures from Zeeman–Doppler images

K. Wood, A. Cameron, J. Donati, 2002, astro-ph/0207522.

Mean Field Model for the Formation of Filament Channels on the Sun

E. Priest, D. Mackay, A. V. Ballegooijen, 2000 .

Using Kepler transit observations to measure stellar spot belt migration rates

D. Mackay, J. Llama, M. Jardine, 2012, 1202.3785.

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

D. Mackay, A. V. Ballegooijen, K. Meyer, 2013 .

Observing the simulations: applying ZDI to 3D non-potential magnetic field simulations

G. Hussain, D. Mackay, A. Vidotto, 2018, Monthly Notices of the Royal Astronomical Society.

Measuring stellar magnetic helicity density

P. Petit, J. Donati, D. Mackay, 2020, Monthly Notices of the Royal Astronomical Society.