New sites for magnetic reconnection
- Visualizations by:
- Tom Bridgman
- Written by:
- Mara Johnson-Groh
- Produced by:
- Genna Duberstein
- View full credits
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.
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.
Credits
Please give credit for this item to:
NASA's Scientific Visualization Studio
Visualizer
- Tom Bridgman (GST) [Lead]
Writer
- Mara Johnson-Groh (Wyle Information Systems) [Lead]
Producer
- Genna Duberstein (ADNET) [Lead]
Technical support
- Ian Jones (ADNET)
- Laurence Schuler (ADNET)
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 setSDO 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 setNote: 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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