Optimization of Saturn paraboloid magnetospheric field model parameters using Cassini equatorial magnetic field data

The paraboloid model of Saturn's magnetosphere describes the magnetic field as being due to the sum of contributions from the internal field of the planet, the ring current, and the tail current, all contained by surface currents inside a magnetopause boundary which is taken to be a paraboloid...

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Bibliographic Details
Published in:	Annales geophysicae (1988) Vol. 34; no. 7; pp. 641 - 656
Main Authors:	Belenkaya, Elena S., Kalegaev, Vladimir V., Cowley, Stanley W. H., Provan, Gabrielle, Blokhina, Marina S., Barinov, Oleg G., Kirillov, Alexander A., Grigoryan, Maria S.
Format:	Journal Article
Language:	English
Published:	Katlenburg-Lindau Copernicus GmbH 26.07.2016 Copernicus Publications
Subjects:	Analysis Approximation Auroral oval Data Dynamic pressure Geomagnetic fields Ionosphere Magnetic field Magnetic fields Magnetic flux Magnetopause Magnetosphere Mapping Mathematical models Optimization Parabolic bodies Parameters Planetary magnetic fields Planetary magnetospheres Planets Plasma Prediction models Ring currents Saturn Saturn ionosphere Saturn magnetosphere Solar wind Spacecraft Surface currents
ISSN:	1432-0576, 0992-7689, 1432-0576
Online Access:	Get full text
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