Multiple CMEs of October 2013
In this research model run, the Sun has launched three coronal mass ejections (CMEs) which may merge into a single front as it expands into the solar system. These events are sometimes called 'cannibal' CMEs.
This model run is based on estimated parameters from solar events of October 23-24, 2013
Movie with research run of three CMEs merging into one.
This color table represents how displaying each of the three variables as separate red, green, and blue color ramps combine to identify characteristics in the solar wind and CME.
The mass density in atomic mass units (AMUs) per cubic centimeter. 1 AMU/cc corresponds to 1 hydrogen ion or atom per cc.
Plasma temperture scale, in Kelvin.
Credits
Please give credit for this item to:
NASA's Goddard Space Flight Center Scientific Visualization Studio, the Space Weather Research Center (SWRC) and the Community-Coordinated Modeling Center (CCMC), Enlil and Dusan Odstrcil (GMU).
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Animator
- Tom Bridgman (Global Science and Technology, Inc.)
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Producer
- Genna Duberstein (USRA)
Release date
This page was originally published on Monday, November 4, 2013.
This page was last updated on Wednesday, May 3, 2023 at 1:51 PM EDT.
Series
This page can be found in the following series:Datasets used
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Enlil Heliospheric Model (Enlil Heliospheric Model)
ID: 685MHD solar wind simulation
See all pages that use this dataset -
DE421 (JPL DE421)
ID: 752Planetary ephemerides
This dataset can be found at: http://ssd.jpl.nasa.gov/?ephemerides#planets
See all pages that use this dataset
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