Results 171 to 180 of about 23,056 (219)

Observation of super-Alfvénic slippage of reconnecting magnetic field lines on the Sun. [PDF]

Nat Astron
Lörinčík J, Dudík J, Sainz Dalda A, Aulanier G, Polito V, De Pontieu B.   +5 more
europepmc   +1 more source

Eruption-Related Ultraviolet Irradiance Enhancements Associated with Flares. [PDF]

Sol Phys
Majury L, Dominique M, Milligan R, Talpeanu DC, Dammasch I, Berghmans D.   +5 more
europepmc   +1 more source

Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
europepmc   +1 more source

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Magnetic Reconnection in the Solar Wind

Space Science Reviews, 2011
It is only within the last 5 years that we have learned how to recognize the unambiguous signature of magnetic reconnection in the solar wind in the form of roughly Alfvenic accelerated plasma flows embedded within bifurcated magnetic field reversal regions (current sheets).
J T Gosling
openaire   +3 more sources

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
openaire   +1 more source

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
openaire   +1 more source

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
openaire   +1 more source

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
openaire   +1 more source