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December 6, 2024

Switchbacks: Solar jets may hold the key for understanding complete magnetic field reversals

Simulation domain and magnetic topology. Top left: 3D volume of the domain of the simulation with the root blocks of the grid. Bottom left: A 2D cross section at constant angle of ϕ = 0° of the velocity color at t = 5500 s. This snapshot highlights the spatial distribution of the velocity. The grid block boundaries are delineated by gray lines. Each block contains 8 × 8 × 8 cells. Right: Initial magnetic topological structure. The isosurface of plasma β = 20 (red spheroid) indicates the location of the 3D magnetic null point. Magnetic field lines of distinct connectivity bounding the separatrix surface are represented, either closed (white field lines) or open to the heliosphere (blue field lines). Credit: Astronomy & Astrophysics (2024). DOI: 10.1051/0004-6361/202452019
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Simulation domain and magnetic topology. Top left: 3D volume of the domain of the simulation with the root blocks of the grid. Bottom left: A 2D cross section at constant angle of ϕ = 0° of the velocity color at t = 5500 s. This snapshot highlights the spatial distribution of the velocity. The grid block boundaries are delineated by gray lines. Each block contains 8 × 8 × 8 cells. Right: Initial magnetic topological structure. The isosurface of plasma β = 20 (red spheroid) indicates the location of the 3D magnetic null point. Magnetic field lines of distinct connectivity bounding the separatrix surface are represented, either closed (white field lines) or open to the heliosphere (blue field lines). Credit: Astronomy & Astrophysics (2024). DOI: 10.1051/0004-6361/202452019

NASA's Parker Solar Probe mission has detected magnetic distortions in solar wind, known as switchbacks. To better understand these phenomena, whose origins remain uncertain, a study was conducted by a network of collaborators. This study, published in the journal , reveals that solar jets can create similar disturbances without causing a complete reversal of the magnetic field.

NASA's Parker Solar Probe mission revealed the presence of switchbacks, sudden and rapid reversals of the magnetic field in the solar wind. These peculiar phenomena, rarely observed near Earth, have captivated the scientific community due to their enigmatic origins. A leading theory suggests that switchbacks originate from solar jets, which are ubiquitous in the lower atmosphere of the sun.

To investigate their origins, a team of researchers from LPP, LPC2E, FSLAC, the University of Dundee and Durham University conducted 3D to replicate plasma behavior in the sun's atmosphere. These simulations modeled solar jets and studied their propagation in .

By adjusting such as pressure, temperature, and magnetic field strength, the researchers recreated the diversity of solar atmospheres observed. They then analyzed the in a manner similar to the instruments aboard the Parker Solar Probe, identifying magnetic field distortions reminiscent of switchbacks.

Their findings reveal that solar jets can produce magnetic distortions similar to switchbacks, although complete magnetic field reversals were not observed. This suggests that additional solar atmospheric phenomena, interacting with solar jets, may be responsible for switchbacks with total magnetic field reversals. These results encourage further research to unravel these complex mechanisms.

More information: J. Touresse et al, Propagation of untwisting solar jets from the low-beta corona into the super-Alfvénic wind: Testing a solar origin scenario for switchbacks, Astronomy & Astrophysics (2024).

Journal information: Astronomy & Astrophysics

Provided by Sorbonne University

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