Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
School of Mathematics and Statistics, University of Sheffield
Professor of Applied Mathematics and Solar Physics at the University of Sheffield.
SP2RC, Department of Applied Mathematics, University of Sheffield, Sheffield S3 7RH, UK of Applied Mathematics, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK Mary and Westfield College, London, United Kingdom
Space and Atmospheric Physics Group, Blackett Laboratory, Imperial College, London SW7 2BW, UK
Imperial College of Science, Technology and Medicine, London
Astronomy Unit, School of Mathematical Sciences, Queen Mary & Westfield College, Mile End Road, London E1 4NS
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000
Space and Atmospheric Physics, Blackett Laboratory, Imperial College, Prince Consort Road, London SW7 2BW, England, UK
Queen Mary and Westfield College, London, UK
Professor of Physics at Imperial College London. From September 2004 he will be Professor of Applied Mathematics and Solar Physics at the University of Sheffield
Space and Atmospheric Physics Group, The Blackett Laboratory, Imperial College, London, UK
Department of Physics, Imperial College, London, England
QMW
Sheffield, UK
Department of Applied Mathematics, University of Sheffield, Department of Applied Maths University of Sheffield Hicks Building Hounsfield Road, Sheffield, S3 7RH United Kingdom and Atmospheric Physics Group, The Blackett Laboratory, Imperial College, London SW7 2BW
Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield College, Mile End Road, London E1 4NS, UK of London, London, UK
Department of Applied Mathematics, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK.
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA;
A comparison of methods for inverting helioseismic data
A Comparison of Solar p-Mode Parameters from MDI and GONG: Mode Frequencies and Structure Inversions
A Comparison of Solar p-Mode Parameters from the Michelson Doppler Imager and the Global Oscillation Network Group: Splitting Coefficients and Rotation Inversions
A Hands-On IDL Program for Helioseismic Inversion
A Measurement of the Rotation Rate in the Deep Solar Interior
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