Physics – Space Physics
Scientist
Physics
Space Physics
Scientist
Reading University
Center for Space Physics, Boston University, Boston, Massachusetts, USA
Center for Space Physics, Boston University, 725 Commonwealth Ave, Boston, MA 02215, USA University Center for Space Physics, 725 Commonwealth Avenue, Boston, MA 02215, USA Environment Physics Group, Department of Meteorology, University of Reading, Earley Gate; Space and Atmospheric Physics, Imperial College London
Space and Atmospheric Physics Group, Blackett Laboratory, Imperial College London, London, UK
Department of Meteorology, University of Reading, Reading, UK
University of Reading, Reading, United Kingdom; Environment Physics Group, Reading University, Reading, United Kingdom; College London, Space and Atmospheric Physics, United Kingdom
Center for Space Physics, Boston University, Center for Integrated Space Weather Modeling 725 Commonwealth Ave, Boston, MA 02215, USA for Space Physics, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA University, Center for Space Physics, 725 Commonwealth Avenue, Boston, MA 02215, USA University, Center for Space Physics 725 Commonwealth Ave, Boston, MA 02215, USA College London, Space and Atmospheric Physics, Prince Consort Road, London, SW7 2BZ, United Kingdom
Space and Atmospheric Physics, The Blackett Laboratory, Imperial College London
Space Environment Physic Group, University of Reading, Earley Gate, P.O. Box 243, Reading RG6 6BB, UK; The Blackett Laboratory, Imperial College London, Prince Consort Road London SW7 2BZ, UK
Imperial College London, Space an Atmospheric Physics, The Blackett Laboratory, Imperial College London, London, SW7 2AZ, United Kingdom
Space and Atmospheric Physics, Imperial College London, Prince Consort Road, London, SW7 2
A kinematically distorted flux rope model for magnetic clouds
Accretion not Diversion One way ICME-sheaths differ from planetary magnetosheaths
Ambient solar wind's effect on ICME transit times
An event-based approach to validating solar wind speed predictions: High-speed enhancements in the Wang-Sheeley-Arge model
Analysis of the magnetic field discontinuity at the potential field source surface and Schatten Current Sheet interface in the Wang-Sheeley-Arge model
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