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About this work
Introduction
Locating the Earth’s magnetopause through X-ray imaging
Introduction
Earth’s Magnetopause
Detecting the magnetopause
Previous work: Fitting methods
Tangent Hypothesis
Extracting the magnetopause surface from the simulation
LaTeP model: Emissivity cube
Shue model fitted to slices
Radial extraction of full magnetopause
Fitting models to surface
Extracting the magnetopause from the MHD emissivity
Extracting the maximum intensity curve from the image
Image processing
Characterizing the tangent hypothesis
Projecting the surface
Results: Characterizing the Tangent Hypothesis
Tangent Fitting
Tangent Fitting
The method
Benchmarking the fitting method
Discussion and Future developments
Bibliography
Repository
Open issue
Index