Calculation by a Moment Technique of the Perturbation of the Geomagnetic Field by the Solar Wind

Calculation by a Moment Technique of the Perturbation of the Geomagnetic Field by the Solar Wind

<p>An iterative method is developed by which one can calculate approximately the boundary of a magnetic field confined by a plasma. This method consists essentially of varying an assumed surface until the magnetic multipole moments of the currents, which would flow on that surface to bala...

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Bibliographic Details
Main Author: Midgley, James Eardley
Format: Others
Published: 1963
Online Access:https://thesis.library.caltech.edu/7038/3/Midgley_je_1963ocr.pdf
Midgley, James Eardley (1963) Calculation by a Moment Technique of the Perturbation of the Geomagnetic Field by the Solar Wind. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/F6XJ-4H41. https://resolver.caltech.edu/CaltechTHESIS:05172012-071917019 <https://resolver.caltech.edu/CaltechTHESIS:05172012-071917019>

Internet

https://thesis.library.caltech.edu/7038/3/Midgley_je_1963ocr.pdf
Midgley, James Eardley (1963) Calculation by a Moment Technique of the Perturbation of the Geomagnetic Field by the Solar Wind. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/F6XJ-4H41. https://resolver.caltech.edu/CaltechTHESIS:05172012-071917019 <https://resolver.caltech.edu/CaltechTHESIS:05172012-071917019>

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