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Evidence of Magnetic Reconnection in Ganymede's Wake Region From Juno. [PDF]

J Geophys Res Space Phys
Joseph J, Kurth WS, Sulaiman AH, Connerney JEP, Allegrini F, Duling S, Clark G, Faden JB, Piker CW, Jaynes AN, Mauk BH, Bolton SJ.   +11 more
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Magnetic reconnection in solar coronal loops

Advances in Space Research, 1997
Abstract Simulations of the evolution of kink modes in line-tied coronal loops are presented which demonstrate the occurrence of magnetic reconnection in the non-linear stage of the instability. In loops which do not carry a net axial current (and are confined by a potential purely axial field) the reconnection is limited to the initial current ...
G Einaudi, R Lionello, M Velli
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Turbulent magnetic reconnection in the solar wind

2023
Turbulent magnetic reconnection was observed in the magnetotail and the magnetopause. In turbulent magnetic reconnection, the diffusion region is filled with a number of filamentary currents primarily carried by the electrons and some flux ropes. These dynamic filamentary currents constitute a kind of three-dimensional network in the diffusion region ...
Rongsheng Wang, Xinmin Li, Shimou Wang, Quanming Lu, San Lu, Walter Gonzalez   +5 more
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Solar Flares and Magnetic Reconnection Experiments

Physica Scripta, 1984
On the basis of dimensionless parameters a comparison has been made between the solar flares phenomena and special laboratory experiments.
S V Bulanov, V A Dogiel, A G Frank
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Heating the Solar Corona by Magnetic Reconnection

Astrophysics and Space Science, 1998
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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Solar coronal heating by forced magnetic reconnection: Multiple reconnection events

Physics of Plasmas, 2005
Magnetic reconnection is a strong candidate for a coronal heating mechanism, and heating by forced magnetic reconnection is investigated here. Two dimensional, nonlinear magnetohydrodynamic simulations are used to investigate forced magnetic reconnection in a compressible plasma. The reconnection occurs when a sheared force-free field is perturbed by a
Rekha Jain, Philippa Browning, K. Kusano
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Magnetic reconnection in solar flares

Geophysical & Astrophysical Fluid Dynamics, 1991
The magnetic energy stored in the corona is the only plausible source for the energy released during large solar flares. During the last 20 years most theoretical work has concentrated on models which store magnetic energy in the corona in the form of electrical currents, and a major goal of present day research is to understand how these currents are ...
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Magnetic reconnection and some solar applications

Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences, 2000
Magnetic reconnection is a fundamental plasma–physics process that is of great importance for the Sun, the Earth9s magnetosphere and all astrophysical objects which have magnetic fields. It is a process central to the generation of magnetic fields in stars and also plays a major role in the heating of solar and stellar coronae.
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Solar magnetic reconnection seen in detail

Physics Today, 2013
New observations provide the most complete picture yet for the most energetic explosions in the solar system.
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Solar Flares and Magnetic Reconnection

2005
Abstract Recent studies by the author and his colleagues on solar flares based on the magnetic reconnection model are reviewed. The studies have been done mainly by using the data sets of space-craft observations and super-computer simulations. The covered topics are an EUV observation of reconnection inflows, MHD simulations of the reconnection ...
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