Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
University of St Andrews
School of Mathematics & Statistics, University of St Andrews, North Haugh, St Andrews, Fife, KY16 9SS, UK of Mathematical and Computational Sciences, University of St. Andrews, North Haugh, St. Andrews, Fife, KY16 9SS, Scotland, UK
School of Mathematics and Statistics, University of St. Andrews, St. Andrews KY16 9SS, UK University, St. Andrews, Scotland
School of Mathematics and Statistics, The University of St Andrews, St Andrews, Fife KY16 9SS, UK
School of Mathematics and Statistics, University of St Andrews, North Haugh, St Andrews, Fife, KY16 9SS, Scotland
Mathematical Institute, U. St Andrews, Scotland
University of St. Andrews, United Kingdom
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, Saint Andrews, UK
School of Mathematics and Statistics, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS
Stanford University
Mathematical Institute, University of St Andrews, North Haugh, St Andrews, Fife, KY16 9SS, Scotland
Saint Andrews Univ., Saint Andrews, UK
School of Mathematical and Computational Sciences, University of St. Andrews, North Haugh, St. Andrews, Fife, KY16 9SS, Scotland
University of St. Andrews, Scotland, KY, UK
Institute of Mathematics, University of St Andrews, St Andrews, KY16 9SS, UK
School of Mathematics and Statistics, University of St Andrews
University of St Andrews, School of Mathematics and Statistics, University of St Andrews, St Andrews, Fife, KY15 7PB, United Kingdom of Mathematics and Statistics, St. Andrews University, St. Andrews, KY16 9S, United Kingdom of Mathematics and Statistics, University of St Andrews, The No
3D Magnetic Reconnection
A converging flux model of an X-ray bright point and an associated canceling magnetic feature
A model for X-ray bright points due to unequal cancelling flux sources
A model of the Solar Magnetic Carpet
A new view of quiet-Sun topology from Hinode/SOT
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Profile ID: LFWR-SCP-P-36114