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Trinity College Dublin, The University of Dublin

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Research Interests

The image above was created using all the titles of my publications (as of 04.Mar.2015) using

Stellar Winds

Solar-like stars (main sequence and pre-main sequence) & low-mass stars: magnetised coronal winds, rotating outflows, structure of the coronal magnetic field, angular momentum loss, magnetic interaction between planets and the host star, accretion disks.

Exoplanetary Magnetic Fields

Formation of bow shocks due to magnetic interaction between planets and the host star. Radio emission through electron-cyclotron maser instability.

Magnetohydrodynamics Waves

Cool supergiant stars: models of winds driven by Alfven waves, wind heating by dissipation of Alfven waves, charged dust-wave interaction.

Magnetohydrodynamics Numerical Simulations

Three-dimensional simulations, time-dependent effects, adaptive mesh refinement.