File:Ganymede field.svg
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DescriptionGanymede field.svg | Magnetic field of Ganymede. Calculated using data from Gallileo's second encounter to the moon at September 6th 1996 (superposition model with 120nT homogenous field and equatorial field strength of 720nT for the moon's own dipole field). The co-rotating Ganymede-centered reference system is such that the x-axis points towards Jupiter, the z-axis is the common spin axes of Jupiter, Ganymede and its orbit. The y-axis is suppressed and shows in direction of Ganymede's orbital motion. The green line - the separatrix - seperates regions of magnetic field lines which a) go from moon to moon, b) from moon to planet or c) from planet to planet. |
Date | 4 August 2007 (upload date) |
Source | Own work |
Author | CWitte |
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:45, 4 August 2007 | 1,200 × 800 (47 KB) | CWitte (talk | contribs) | better arrows | |
12:19, 4 August 2007 | 1,800 × 1,200 (144 KB) | CWitte (talk | contribs) | minor things and license | ||
11:46, 4 August 2007 | 2,400 × 3,600 (41 KB) | CWitte (talk | contribs) | {{Information |Description=Magnetic field of Ganymede. Calculated using data from Gallileo's second encounter to the moon at September 6th 1996 (superposition model with 120nT homogenous field and equatorial field strength of 720nT for the moon's own dipo |
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