A newer version of this visualization is available.
The Solar 'Constant' - Faculae vs. Sunspots
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- Visualizations by:
- Tom Bridgman
- View full credits
Three views of the Sun showing different levels of solar activity. The color table has been altered to enhance the appearance of the faculae (white regions) which are hotter than sunspots (red-black regions) and whose greater total area contribute to increasing the solar flux reaching the Earth.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio. Source data courtesy of HAO & NSO PSPT project team. HAO is a division of the National Center for Atmospheric Research which is supported by the National Science Foundation.Special thanks to Vanessa George (University of Colorado/LASP) and Randy Meisner(Michigan State University)
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Animator
- Tom Bridgman (Global Science and Technology, Inc.) [Lead]
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Scientists
- Gary Rottman (University of Colorado/LASP)
- Robert F. Cahalan (NASA/GSFC)
- William R. Ochs (NASA/GSFC)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Datasets used in this visualization
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PSPT
ID: 80 -
SORCE
ID: 97The SORCE mission (launched January 23, 2003) will study the variability of the Sun and its impact on the Earth"s Climate.
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Newer Versions
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ID: 4892
VisualizationFaculae and Sunspots at Solar Maximum and Solar Minimum