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Journal ArticleDOI

A thruster using magnetic reconnection to create a high-speed plasma jet

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TLDR
In this paper, a pulsed magnetic reconnection thruster consisting of two parallel-connected slit coaxial tubes was constructed and operated in argon plasma produced by RF energy at 13.56 MHz.
Abstract
Plasma thrusters propel spacecraft by the application of Lorentz forces to ionized propellants. Despite evidence that Lorentz forces resulting from magnetic reconnection in solar flares and Earth's magnetopause produce jets of energetic particles, magnetic reconnection has only recently been considered as a means of accelerating plasma in a thruster. Based on theoretical principles, a pulsed magnetic reconnection thruster consisting of two parallel-connected slit coaxial tubes was constructed. The thruster was operated in argon plasma produced by RF energy at 13.56 MHz. A 1.0 ms current pulse of up to 1500 A was applied to the tubes. Three results provide evidence for magnetic reconnection. (1) The production of high-energy electrons resembling the outflow that is observed in the reconnection of field lines in solar flares and in laboratory experiments. (2) The high-energy electron current coincided with the rise of the magnetic field in the thruster and was followed by a large ion current. (3) In accordance with known physics of magnetic reconnection, ion currents were found to increase as the plasma became less collisional. The Alfven speed of the outflowing ions was calculated to be 8.48 × 103 m s− 1 corresponding to an Isp of 860 s.

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Citations
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Journal Article

Progress in Understanding Magnetic Reconnection in Laboratory and Space Astrophysical Plasmas

TL;DR: Yamada et al. as mentioned in this paper reviewed the progress in understanding the fundamental physics of magnetic reconnection, focusing on significant results in the past decade from dedicated laboratory experiments, numerical simulations, and space astrophysical observations.
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Magnetic Reconnection in the Space Sciences: Past, Present, and Future

TL;DR: Magnetic reconnection is a key energy conversion and transport process in space and in the laboratory as discussed by the authors, which facilitates energy conversion over dimensions of, in some cases, hundreds of Earth radii.
Journal ArticleDOI

An Alfvenic reconnecting plasmoid thruster

TL;DR: In this article, a new concept for generation of thrust for space propulsion is introduced, which utilizes a current-sheet instability to spontaneously and continuously create plasmoids via magnetic reconnection, and the generated low-temperature plasma is simulated in a global annular geometry using the extended magnetohydrodynamic model.
References
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Journal ArticleDOI

Sweet's mechanism for merging magnetic fields in conducting fluids

TL;DR: In this paper, it was shown that two oppositely directed sunspot fields with scales of 104 km could be merged by Sweet's mechanism, if shoved firmly together, in about two weeks; their normal interdiffusion time would be of the order of 600 years.
Book

Magnetic Reconnection: MHD Theory and Applications

TL;DR: Magnetic reconnection is at the core of many dynamic phenomena in the universe, such as solar flares, geomagnetic substorms and tokamak disruptions as discussed by the authors.
Journal ArticleDOI

Role of electron physics in the development of turbulent magnetic reconnection in collisionless plasmas

TL;DR: In this article, Petaflop-scale simulations of the evolution of turbulent magnetic reconnection in a three-dimensional plasma indicate that it proceeds in a way that is dramatically different from classical theory.
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