Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Centre for Fusion, Space and Astrophysics, Department of Physics, University of Warwick, Coventry CV4 7AL, UK
University of Warwick, Coventry, UK
Mullard Space Science Laboratory, University College London, Surrey, UK
Centre for Fusion, Space and Astrophysics, Department of Physics, University of Warwick, Coventry CV4 7AL, UK; Mullard Space Science Laboratory, University College London, Dorking, UK
Physics, University of Warwick, Coventry, United Kingdom;
Belgian Institute for Space Aeronomy;, University of Warwick
University of Warwick, Center for Fusion, Space and Astrophysics, Department of Physics, Coventry, United Kingdom
School of Mathematical and Computational Sciences, University of St Andrews, St Andrews KY16 9SS, Scotland
Department of Physics, University of Warwick; Mullard Space Science Laboratory, University College London
Department of Physics, University of Warwick, Coventry CV4 7AL, UK for Fusion, Space and Astrophysics, Department of PhysicsUniversity of Warwick, Coventry, CV4 7AL, UK
School of Mathematics and Statistics, University of St. Andrews, Scotland, UK
School of Mathematics and Statistics, University of St. Andrews, Scotland, UK ; Center Plasma Astrophysics, K. U. Leuven, Celestijnenlaan 200B, 3001 Heverlee, Belgium Space Science Laboratory, UCL, Holmbury St. Mary, Dorking, RH5 6NT, United Kingdom
CFSA, Department of Physics, University of Warwick, Coventry CV4 7AL, UK
Mullard Space Science Laboratory, University College London; Centre for Fusion, Space and Astrophysics, Department of Physics, University of Warwick
Center for Fusion, Space and Astrophysics, Department of Physics, University of Warwick, Coventry, UK
Physics, University of Warwick, Coventry, United Kingdom
Automated detection and 3D reconstruction of EUV prominences
Automated Detection of EUV Prominences
Cluster observations of the mid-altitude cusp under strong northward Interplanetary Magnetic Field
Cluster observations of the mid-altitude cusp under strong northward Interplanetary Magnetic Field
Damped large amplitude transverse oscillations in an EUV solar prominence, triggered by large-scale transient coronal waves
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