2024
DOI: 10.1063/5.0177975
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Observation of rapid flux coalescence in merging field-reversed configurations

T. Asai,
T. Seki,
D. Kobayashi
et al.

Abstract: Rapid magnetic reconnection was experimentally observed to occur within a microsecond timescale, leading to the field-reversed configuration (FRC) comprising a single closed magnetic field structure. The compressibility of the plasma within the FRC played a crucial role in accelerating the coalescence process, making it considerably faster than the resistive process. A strong similarity between the observed experimental results and those of the coalescence of solar flare loops indicates that astrophysical phen… Show more

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“…These include the high-beta characteristics of the FRC, associated kinetic effects, and the formation of shock waves from collisions at high speeds that surpass the Alfvén velocity. Among these effects, the rapid reconnection process [38], which is linked to the compressible nature of the FRC formed predominantly by poloidal magnetic fields, resembles the fast reconnection process in solar flares [39,40], which share similar geometric structures and which are explained by current-loop coalescence [41].…”
Section: Discussionmentioning
confidence: 99%
“…These include the high-beta characteristics of the FRC, associated kinetic effects, and the formation of shock waves from collisions at high speeds that surpass the Alfvén velocity. Among these effects, the rapid reconnection process [38], which is linked to the compressible nature of the FRC formed predominantly by poloidal magnetic fields, resembles the fast reconnection process in solar flares [39,40], which share similar geometric structures and which are explained by current-loop coalescence [41].…”
Section: Discussionmentioning
confidence: 99%