User:Tohline/Appendix/Ramblings/Saturn

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Saturn

Whitworth's (1981) Isothermal Free-Energy Surface
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Hexagon Storm

Image on the Right: obtained from this NASA/JPL site; image on the Left: obtained from this NASA Newsletter. See also the wikipedia page titled, Saturn's hexagon.

Casini image

Image of Saturn's Hexagon Storm

Post Cassini

Binary Mass-Transfer

Several key references:


MFTD (2007)
Model Q0.4D
Animation: video4.mpg
(link is in caption of their Figure 3)

MFSCFEDT (2017)
Model Q0.4P_S1
Animation: apjsaa5bdef26_video.mpg
(link is in caption of their Figure 26)

MFSCFEDT (2017)
Model Q0.5P_G1
Animation: apjsaa5bdef21_video.mpg
(link is in caption of their Figure 21)

Q04DcroppedD.png Q0.4P S1croppedD.png Q0.5P G1croppedD.png
Q04D squareD.png Q0.4P S1 squareD.png Q0.5P G1 squareD.png
Q04D triangleD.png Q0.4P S1 triangleD.png Q0.5P G1 triangleD.png
The evolution identified here as Model Q0.5P_G1 was first discussed in §5.2 of DMTF (2006), wherein it was identified as Model Q0.5-Da; the caption to Figure 7 of that paper contains a link to an (mpeg_file = video3-2.mpg) animation that presents a 3D rendering of this model's evolution.

Related Discussions

Whitworth's (1981) Isothermal Free-Energy Surface

© 2014 - 2021 by Joel E. Tohline
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Recommended citation:   Tohline, Joel E. (2021), The Structure, Stability, & Dynamics of Self-Gravitating Fluids, a (MediaWiki-based) Vistrails.org publication, https://www.vistrails.org/index.php/User:Tohline/citation