Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
British Antarctic Survey, Cambridge, UK
British Antarctic Survey, High Cross Madingley Road, Cambridge, CB3 0ET United Kingdom
Imperial College of Science and Technology, London, England
Natural Complexity Project British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET United Kingdom
Imperial College of Science, Technology, and Medicine, London, England
Imperial College of Science, Technology, and Medicine, London, United Kingdom
Physical Sciences Division, British Antarctic Survey, Natural Environment Research Council, Cambridge, UK
British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET, United Kingdom
British Antarctic Survey, Cambridge, United Kingdom
NERC, British Antarctic Survey, Cambridge, England
Imperial College, London, UK
Johns Hopkins University, Laurel, MD
British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 9JA United Kingdom
British Antarctic Survey, High Cross Madingley Road, Cambridge, Cam CB3 0ET United Kingdom
Imperial College of Science, Technology and Medicine, London, England
British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET United Kingdom
British Antarctic Survey, Madingley Rd, Cambridge, CB3 OET United Kingdom
British Antarctic Survey, Madingley Road, Cambridge, CB3 0ET, UK
NERC, British Antarctic Survey, Cambridge, United Kingdom
University of Leicester, Leicester, UK
Natural Complexity, British Antarctic Survey, Cambridge, United Kingdom
British Antarctic Survey, Cambridge, U.K.
British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET, UK
A comparison of midlatitude Pi 2 pulsations and geostationary orbit particle injections as substorm indicators
A linear perturbation analysis of magnetopause motion in the Newton-Busemann limit
A minimal substorm model that explains the observed statistical distribution of times between substorms
A statistical analysis of ionospheric velocity and magnetic field power spectra at the time of pulsed ionospheric flows
A statistical comparison of SuperDARN spectral width boundaries and DMSP particle precipitation boundaries in the morning sector ionosphere
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Profile ID: LFWR-SCP-P-184326