New sites for magnetic reconnection

  • Released Tuesday, December 17, 2019
  • ID: 4761

HD and UHD movie views of the plasma flowing along magnetic fields lines visible at 171Å.

This sequence of solar imagery from Solar Dynamics Observatory (SDO) reveals some observational evidence of a previously theorized alternative driver of magnetic reconnection.

Plasma flows tracing the magnetic field configuration (AIA 171Å imagery), and a nearby prominence (AIA 304Å imagery) illustrate this interchange of matter and energy. The primary event of interest occurs just above the active region on the left limb of the Sun between 14:00 and 15:00 hours UT on May 3, 2012.

HD and UHD movie views of the solar prominence visible at 304Å.

4Kx4K frames of the plasma flowing along magnetic fields lines visible at 171Å.

4Kx4K frames of the solar prominence visible at 304Å.

Credits

Please give credit for this item to:
NASA's Scientific Visualization Studio

Missions

This visualization is related to the following missions:

Datasets used in this visualization

SDO AIA 171 (A.K.A. 171 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER 2012-05-03T11:00 to 2012-05-03T17:00

Dataset can be found at: http://jsoc.stanford.edu/

See more visualizations using this data set
SDO AIA 304 (A.K.A. 304 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER 2012-05-03T11:00 to 2012-05-03T17:00

Dataset can be found at: http://jsoc.stanford.edu/

See more visualizations using this data set

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.

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