The CME, traveling at 850 miles per hour, headed straight towards Earth and struck Earth's magnetosphere the afternoon of July 14, 2012. The plasma of the CME carried a complex magnetic field, most of it directed southward. But Earth's magnetic field is directed nortward at the outer boundary of the magnetopause. When these two different magnetic fields merge, reconnection can take place, pumping energy from the magnetic fields into energies of the plasma particles.
This visualization was generated using data from a BATS-R-US simulation run which was initialized using data from the ACE spacecraft and Earth's magnetic field configuration at the time. The Sun is to the left in these simulations.
Each image frame corresponds to 2 minutes of elapsed time.
Density data is plotted in a 2-dimensional plane sliced through the 3-D dataset. Red is high density,and blue is low density (see color bar for details).
The magnetic field lines are 3-dimensional structures which is more apparent in the oblique and polar views.
As the magnetosphere responses to the CME, we see field lines forming complex structures, and radically change directions. The field has significant structure changes on the sunward side, and the night side of Earth, where reconnection-type events are occurring.
Field line colors represent details of where these structures are connected: - White field lines are closed - Green field lines are open from north geographic (south magnetic) pole - Red field lines are open from south geographic (north magnetic) pole - Cyan field lines are seeded in the magnetotail. Some are open and some closed. - Magenta field lines are seeded ahead of the magnetopause.
Please give credit for this item to: NASA's Scientific Visualization Studio, the Space Weather Research Center (SWRC), the Community-Coordinated Modeling Center (CCMC) and the Space Weather Modeling Framework (SWMF).
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BATS-R-US Magnetosphere Model
Model - Community Coordinated Modeling Center (CCMC) - 2012-07-14T00:00:00 - 2012-07-17T00:00:00