SC
Member Since 1985
Sandra C. Chapman
Professor of Physics, University of Warwick
Professional Experience
University of Warwick
Professor of Physics
1995 - Present
University of Warwick
Education
Imperial College London
Doctorate
1985
Publications
Statistical Characteristics of Total Electron Content Intensifications on Global Ionospheric Maps
Global ionospheric total electron content (TEC) maps exhibit TEC intensifications and depletions of various sizes and shapes. Characterizing key fe...
January 24, 2024
Variation of Geomagnetic Index Empirical Distribution and Bu...
January 18, 2022
Wavelet and Network Analysis of Magnetic Field Variation and...
September 09, 2021
AGU Abstracts
What does complexity science mean for Heliophysics? A living history and demonstrating a new paradigm in the study of GICs
UNDERSTANDING GEOMAGNETICALLY INDUCED CURRENTS AND THEIR IMPACT ON TECHNOLOGY II ORAL
spa-magnetospheric physics | 14 december 2023
Ryan M. McGranaghan, Lauren Orr, Sandra C. Chapman
Heliophysics processes span at least 15 orders of magnitude in space and another 15 in time, and its reaches go well beyond our own solar system and E...
View Abstract
Beyond Hasselmann and Leith: The Challenge of non-Markovian (and Fractional) Stochastic Climate Modelling
40 YEARS OF ATMOSPHERIC SCALING: FROM CLOUDS TO CLIMATE VARIABILITY ACROSS SCALES I ORAL
nonlinear geophysics | 13 december 2022
Nicholas W. Watkins, Raphael Calel, Sandra C. Chap...
The stochastic energy balance models (SEBMs) pioneered by Hasselmann and Mitchell [1] have long been known to climate scientists to be important aids ...
View Abstract
Magnetic topology of Actively Evolving and Passively Convecting Structures in the Turbulent Solar Wind
REVEALING MULTISCALE PLASMA DYNAMICS AND PROPERTIES OF TURBULENCE IN THREE DIMENSIONS: INSIGHTS FROM MULTI-SPACECRAFT OBSERVATIONS FROM CLUSTER AND MMS TO HELIOSWARM AND BEYOND I ONLINE POSTER DISCUSSION
spa-solar and heliospheric physics | 12 december 2022
Nicholas W. Watkins, Bogdan Hnat, Sandra C. Chapma...
Multipoint in-situ observations of the solar wind are used to identify the magnetic topology and currentdensity of turbulent structures. We find that ...
View Abstract
Check out all of Sandra C. Chapman’s AGU Research!
View All Research Now