Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
MSSL, Holmbury ST. Mary, Holmbury St. Mary, Sur 00000 United Kingdom; DAMPT, University of Cambridge, Department of Applied Maths and Physics, Cambridge, 000000 United Kingdom
DAMTP, Centre for Mathematical Sciences, Wilberforce road Cambridge, CB3 0WA, UK Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK
Mullard Space Science Laboratory, UK
Department of Applied Mathematics and Theoretical Physics, University of Cambridge, UK
Department of Applied Mathematics and Theoretical Physics, The Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 OWA, Cambridge, UK
Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
University College London, MSSL
Solar and Stellar Physics, Mullard Space Science Laboratory, Holmbury St Mary
DAMTP, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA, UK University College London
MSSL, University College London, Holmbury St., Mary Dorking, RH5 6NT, UK
Centre for Astrophysics, University of Central Lancashire, Preston, UK
Mullard Space Science Lab, United Kingdom
University College London, United Kingdom
MSSL, United Kingdom
DAMTP, University of Cambridge, Cambridge, UK
Department of Applied Mathematics and Theoretical PhysicsUniversity of Cambridge, Wilberforce road, Cambridge, CB3 0WA, UK
Centre for Astrophysics, University of Central Lancashire, Preston PR1 2HE UK Univ., United Kingdom
University of Central Lancashire, UK
Department of Applied M
A benchmark study for CHIANTI based on RESIK solar flare spectra
A Different Emission Measure Analysis of AU Mic Flares
A Direct Comparison Between EUV Coronal Flux and Helium Resonance Line Photon Flux from SOHO/CDS Data
A Multi-Wavelength Study of the Compact M1 Flare on October 22, 2002
A Reconnection-driven Rarefaction Wave Model for Coronal Outflows
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