Sun  ID: 4957

Parker Solar Probe: The Origins of Switchbacks

Visualizations by Tom Bridgman Released on December 14, 2021
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Most of the magnetic field measured at Parker during this time is directed sunward (blue field lines and vectors). A switchback occurs when the field changes direction almost 180 degrees for a short period of time. FIELDS instrument magnetic vector data are projected from the spacecraft position as arrows. The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line. The heliospheric magnetic field lines are represented as gold.
For a number of years, solar scientists have known about a phenomenon they called 'switchbacks'. Switchbacks are short-term 'flips' in the polarity of the magnetic field in the outflowing solar wind. Parker Solar Probe has detected these 'switchbacks' (Switchbacks Science: Explaining Parker Solar Probe’s Magnetic Puzzle), which appear to be more plentiful closer to the Sun.

In the visualization above, Parker is passing through a region of inward bound magnetic flux (blue lines). This surrounding field is computed from a running average of the measurements by Parker, which are computing from the individual measurements at Parker's position (arrows projecting from the spacecraft position). For a brief time, these vectors flip direction, in this particular case changing color from blue to white and red, from the surrounding field, which is the signature of a switchback.

Closer to the Sun, the average field lines trace back to coronal structures called pseudostreamers, that are magnetic structures which overlay and connect multiple pole magnetic regions. These regions also appear to correlate with where magnetic flux emerges between supergranule convection cells.
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Most of the magnetic field measured at Parker during this time is directed sunward (blue field lines and vectors). A switchback occurs when the field changes direction almost 180 degrees for a short period of time. FIELDS instrument magnetic vector data are projected from the spacecraft position as arrows. The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line. The heliospheric magnetic field lines are represented as gold.
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A top-down view from the ecliptic pole of the orbit of Parker Solar Probe for Encounter 6. FIELDS instrument magnetic vector data are projected from the spacecraft position with arrows. The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line. The heliospheric magnetic field lines are the gold lines, representing the propagation of the average field measured at Parker, propagated back to the solar photosphere.
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View of FIELDS instrument magnetic data measured at Parker Solar Probe during encounter 6. FIELDS instrument magnetic vector data are projected from the spacecraft position as arrows. The arrows are colored deep blue for sunward vectors, deep red for anti-sunward, and in between for directions off from this line. The heliospheric magnetic field lines are the gold lines, representing the propagation of the average field measured at Parker, propagated back to the solar photosphere.
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A top-down view from the ecliptic pole of the orbit of Parker Solar Probe for Encounter 6.
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A visualization from behind Parker Solar Probe as it approaches the Sun on Encounter 6.
 

Used Elsewhere In

NASA's Parker Solar Probe Touches The Sun For The First Time

Related

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Animation: Origins of Switchbacks
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Visualization Credits

Tom Bridgman (GST): Lead Visualizer
Stuart Bale (University of California, Berkeley): Lead Scientist
Samuel Badman (University of California at Berkeley): Scientist
Joy Ng (KBRwyle): Producer
Mara Johnson-Groh (Wyle Information Systems): Writer
Laurence Schuler (ADNET Systems, Inc.): Technical Support
Ian Jones (ADNET Systems, Inc.): Technical Support
Please give credit for this item to:
NASA's Scientific Visualization Studio

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Mission:
Parker Solar Probe

Data Used:
SPICE Ephemerides also referred to as: SPICE Ephemerides
Ephemeris - NASA/JPL
Satellite and planetary ephemerides
view all stories where this data set is used
Parker Solar Probe/FIELDS also referred to as: FIELDS
University of California at Berkeley
Measurements of electric and magnetic fields and waves.
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.

This item is part of this series:
AGU 2021 - Parker Solar Probe

Keywords:
SVS >> Solar Wind
SVS >> Space Weather
SVS >> Hyperwall
SVS >> Heliophysics
SVS >> Solar Magnetic Field
NASA Science >> Sun
SVS >> Parker Solar Probe