THEMIS Explores the Earth's Bow Shock

  • Released Tuesday, December 11, 2007
View full credits

The solar wind's first contact with the Earth's magnetic field creates a region known as the bow shock, much like the bow wave of a boat moving through the water. This region can also create additional turbulence which generates bursts of explosion-like currents. In this visualization, the orbits of the THEMIS fleet are combined with a 2-D slice from a hybrid magnetosphere simulation which illustrates these turbulent regions in the bow shock. This hybrid magnetosphere simulation treats the slow-moving ions by particle-in-cell computational methods and the faster electrons as a massless fluid. These simulations more accurately represent the magnetospheric physics, enabling a view of turbulent non-linear processes not visible in the simpler magnetohydrodynamic models. In this simulation, the color table is somewhat unusual. In order of increasing density, the colors run from white through violet, blue, green to black.

This movie opens with a view of the five THEMIS satellites (the color dots) moving along their orbits. We then fade in the 2-D data from the Omidi simulation and zoom in to view the turbulence in the region of the bow shock.

Opening view above the north geographic pole of the five THEMIS satellites in orbit around the Earth.

Opening view above the north geographic pole of the five THEMIS satellites in orbit around the Earth.

Moving down near the equatorial plane, the five satellite are near the apogee of their orbits.

Moving down near the equatorial plane, the five satellite are near the apogee of their orbits.

Push in to a view of the satellites in the turbulent region near the bow shock. The 'bubbles' of violet and white surrounded by green and black illustrate broad the range of particle densities in this turbulence.

Push in to a view of the satellites in the turbulent region near the bow shock. The 'bubbles' of violet and white surrounded by green and black illustrate broad the range of particle densities in this turbulence.

A later view of the turbulence which changes significantly on time scales of seconds.

A later view of the turbulence which changes significantly on time scales of seconds.

For More Information

See http://www.nasa.gov/mission_pages/themis/auroras/northern_lights.html

Credits

Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio

This page was originally published on Tuesday, December 11, 2007.
This page was last updated on Wednesday, May 3, 2023 at 1:55 PM EDT.

Missions

This page is related to the following missions:

Series

This page can be found in the following series:

Related papers

Omidi, N., 'Formation of cavities in the foreshock' in 'Turbulence and nonlinear processes in astrophysical plasmas'. Editors D. Shaikh and G. Zank. AIP Conference Proceedings 932, 2007.

Omidi, N., 'Formation of cavities in the foreshock' in 'Turbulence and nonlinear processes in astrophysical plasmas'. Editors D. Shaikh and G. Zank. AIP Conference Proceedings 932, 2007.

Datasets used

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.