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27 lip 2018 · In these visualizations, we present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes.
The data it sent back to us showed that Uranus has a very unusual magnetosphere, which indicated that Uranus has a very large obliquity, which means its rotational axis is about 97.9° away from the north direction, with a relative rapid (17.24 hours) daily rotation.
2 paź 2024 · Uranian Magnetosphere. Model GSFC-O 3. Dipole field strength: 0.228 Gauss-Ru 3 Dipole tilt to rotational axis: 58.6 degrees Longitude of tilt: 53.6 degrees Dipole offset: 0.352 Ru Surface (1 Ru) field strength: ~0.1 - 1.0 Gauss. Ru denotes Uranian model radius, here defined to be 25,600 km.
1 lip 2014 · To explain the 2011 HST observations of Uranus' aurora, Cowley proposed a conceptual picture of open magnetic flux tube evolution in Uranus's magnetosphere under near-equinox conditions. We can test the magnetopause reconnection aspects of this concept with our model.
Download scientific diagram | (left) Simulation of Uranus' magnetic field lines, color coded by strength, at a specific instant in time which highlights the magnetic dipole axis tilt,...
22 kwi 2019 · USDZ File (3D Model) NASA explores the unknown in air and space, innovates for the benefit of humanity, and inspires the world through discovery. A 3D model of Uranus.
An animated GIF showing Uranus' magnetic field. The yellow arrow points to the Sun, the light blue arrow marks Uranus' magnetic axis, and the dark blue arrow marks Uranus' rotation axis. Image Credit:
