Flow Field Representation of Jupiter's Great Red Spot
This visualization shows a simple simulated flow field representation of Jupiter's Great Red Spot. The flow field is static (i.e., the wind directions don't change over time).
This visualization was created in support of the Science On a Sphere film called "Largest" which is about Jupiter. These frames were rendered "flat" and are intended to be duplicated several times around the sphere.
Great Red Spot wind flow field simulation
Great Red Spot wind flow field simulation print still
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio
-
Animators
- Greg Shirah (NASA/GSFC)
- Tom Bridgman (Global Science and Technology, Inc.)
-
Video editor
- Victoria Weeks (HTSI)
-
Producer
- Michael Starobin (HTSI)
-
Scientist
- Amy A. Simon (NASA/GSFC)
Release date
This page was originally published on Monday, September 21, 2009.
This page was last updated on Wednesday, May 3, 2023 at 1:54 PM EDT.
Series
This page can be found in the following series:Datasets used
-
[Simulated Jupiter Wind Flow Field]
ID: 641
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.