Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
School of Mathematics and Statistics, University of St Andrews, UK
Saint Andrews, University, Scotland
School of Mathematics and Statistics, University of St. Andrews, North Haugh, St Andrews, Fife KY16 9SS, Scotland
Department of Mathematical Sciences, University of St. Andrews, Fife, KY16 9SS, Scotland
St. Andrews, University, St. Andrews, Scotland
Florence Univ., Italy
School of Mathematics and Statistics, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS, UK
University of St. Andrews, St. Andrews, Scotland, UK
Department of Mathematical and Computational Sciences, University of St Andrews, St Andrews, KY16 9SS, UK
School of Mathematics and Statistics, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS
School of Mathematics and Statistics, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, Scotland Andrews, University, Scotland
Saint Andrews, University, Scotland; Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany
School of Mathematics and Statistics, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS, UK of Mathematics and Statistics, University of St. Andrews, North Haugh, St. Andrews, Fife, KY16 9SS, UK
St. Andrews, Fife, KY16 8YA, UK
Department of Mathematical and Computational Sciences, University of St. Andrews
School of Mathematics and Statistics, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS, UK.
School of Mathematics and Statistics, St Andrews University, St Andrews, Fife KY16 9SS, Scotland
School of Mathematical and Computational Sciences, University of St. Andrews, St. Andrews KY16 9SS, UK
School of Mathematics and Statistics, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK
St. Andrews Univ., United Kingdom
California Univ., Berkeley
School of Mathematics and Statistics, University of St Andrews, North Haugh, St Andrews, KY16 9SS, Scotland
School of Mathematics a
3D MHD Coronal Oscillations About a Magnetic Null Point: Application of WKB Theory
3D MHD Flux Emergence Experiments: Idealised Models and Coronal Interactions
3D MHD Flux Emergence Experiments: Idealized models and coronal interactions
3D simulations identifying the effects of varying the twist and field strength of an emerging flux tube
A complete coronal loop stability analysis in ideal magnetohydrodynamics. II. Force-free cylindrical equilibria
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