Sun  ID: 4639

MMS Sees a New Type of Reconnection

Visualizations by Tom Bridgman Released on May 9, 2018
The Magnetospheric Multiscale (MMS) mission consists of four identical satellites that traverse various regions of Earth's magnetosphere measuring the particles and electric and magnetic field which influence them.

In the turbulent plasma between Earth's magnetopause and bow shock, a region called the magnetosheath, the MMS satellite constellation has measured multiple jets of energetic electrons between magnetic bubbles. This appears to be a new 'flavor' of magnetic reconnection based on electrons and occuring on smaller time and spatial scales than the standard model of magnetic reconnection with ions.

In these data visualizations, the arrows represent the data collected by the spacecraft. To better comprehend changes as the spacecraft moves along, the data are allowed to 'echo' along the spacecraft trail. The length of the vectors represent the relative magnitude of the vector. However, the electron and proton vectors are scaled so equal velocities correspond to vectors of equal magnitude.

  • Magenta represents the direction and magnitude of the magnetic field at the spacecraft position.
  • Green represents the direction and magnitude of the net electric current created by the motion of the electrons and ions measured at the spacecraft position.

The four MMS spacecraft are represented by colored spheres, corresponding to the plotted data lines in the lower graphic
  • MMS1
  • MMS2
  • MMS3
  • MMS4

The clocks on MMS are synchronized for the TAI (International Atomic Time) system provided through the Global Positioning System (GPS) satellites. It provides a high-precision time reference for comparing MMS measurements to other datasets.
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From a wide view of the MMS orbit, this visualization zooms down to the four spacecraft as they move between the magnetopause and bow shock. Along the track of each spacecraft we see the measured magnetic field vectors (magenta arrows) and the measured current vectors (green arrows). The energetic event of interest occurs at clock time of 09:03:54.3 TAI.
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This visualization travels along with the four MMS spacecraft as they move between the magnetopause and bow shock. Along the track of each spacecraft we see the measured magnetic field vectors (magenta arrows) and the measured current vectors (green arrows). This view illustrates the dramatic changes in the magnetic field measurements as the spacecraft travel between the plasma 'bubbles' in this region. The energetic event of interest occurs at clock time of 09:03:54.3 TAI. This version has a lower time resolution (0.15 seconds per frame) so some detail is lost. This visualization is frame-synchronized with the animated graph.
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From a wide view of the MMS orbit, this visualization zooms down to the four spacecraft as they move between the magnetopause and bow shock. Along the track of each spacecraft we see the measured magnetic field vectors (magenta arrows) and the measured current vectors (green arrows). The energetic event of interest occurs at clock time of 09:03:54.3 TAI.
Download Options
From a wide view of the MMS orbit, this visualization zooms down to the four spacecraft as they move between the magnetopause and bow shock. Along the track of each spacecraft we see the measured magnetic field vectors (magenta arrows) and the measured current vectors (green arrows). The energetic event of interest occurs at clock time of 09:03:54.3 TAI.
Download Options
Animated plot of current measured by the MMS spacecraft. This animation is frame-synchronized with the DataTour visualization above. It also plots the data at a higher time-resolution than DataTour. Colors correspond to the spacecraft doing the measurement. Red=MMS1, blue=MMS2, cyan=MMS3, yellow=MMS4.
 

Used Elsewhere In

SVS Demo Reel
NASA Spacecraft Finds New Magnetic Process in Turbulent Space

Related

Data Tour of MMS and Magnetopause Reconnection
Zoom in to MMS and Magnetopause Reconnection
MMS Fly Along with Magnetopause Reconnection

Visualization Credits

Tom Bridgman (GST): Lead Visualizer
Tai Phan (University of California at Berkeley): Lead Scientist
Joy Ng (USRA): Lead Producer
Mara Johnson-Groh (Wyle Information Systems): Lead Writer
Please give credit for this item to:
NASA's Scientific Visualization Studio

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https://svs.gsfc.nasa.gov/4639

Mission:
Magnetospheric Multiscale (MMS)

Data Used:
MMS/FIELDS also referred to as: MMS-FIELDS
Observed Data - 2016-12-09T08:58:54 - 2016-12-09T09:05:00
view all stories where this data set is used
MMS/Fast Plasma Investigation also referred to as: MMS-FPI
Event List - 2016-12-09T08:58:54 - 2016-12-09T09:05:00
view all stories where this data set is used
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.

Keywords:
SVS >> Geomagnetic Field
SVS >> Magnetic Reconnection
SVS >> Plasma
GCMD >> Location >> Magnetosphere (other)
GCMD >> Location >> Bow Shock
GCMD >> Location >> Magnetopause
SVS >> Hyperwall
SVS >> MMS
NASA Science >> Sun

GCMD keywords can be found on the Internet with the following citation: Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version 8.0.0.0.0