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Research Astronomer at the Armagh Observatory. He has long experience in the study of magnetic activity phenomena relating to cool stars; in general. He has experience in (i) the calculation and application of atomic physics to the reduction/interpretation of solar and stellar data, (ii) solar physics (including the reduction and interpretation of sunspot, plage and flare data from several solar space missions (iii) the reduction and interpretation of data relating to cool stars over a vast frequency range, including, X-ray data from EXOSAT, EUVE and GINGA, ultraviolet (IUE, HST), extreme ultraviolet (ROSAT, EUVE), optical (SAAO, INT, WHT, Kitt Peak), infrared (IRAS, UKIRT), millimetre (JCMT, SEST) and radio (VLA, AT, GMRT, EVN). He is involved in the analysis and modelling of numerous solar features, e.g. bright-points, chromospheric oscillations, coronal holes, macro-spicules, etc. Part of this work has also involved simulations of transition region line profiles using non-equilibrium ionization calculations to simulate the fast moving jet features. He has over 260 refereed papers plus 170 non-refereed/conference papers. He is currently involved in the reduction and modelling of data from the space missions SoHO, Hinode and SDO.
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