Results 11 to 20 of about 22,968 (238)

Magnetic Reconnection and Intermittent Turbulence in the Solar Wind [PDF]

open access: yesPhysical Review Letters, 2014
5 pages, 3 figures, submitted to Physical Review ...
K. T. Osman   +7 more
openaire   +6 more sources

A solar filament disconnected by magnetic reconnection [PDF]

open access: yesAstronomy & Astrophysics, 2020
Aims. We aim to study a high-resolution observation of an asymmetric inflow magnetic reconnection between a filament and its surrounding magnetic loops in active region NOAA 12436 on 2015 October 23. Methods. We analyzed the multiband observations of the magnetic reconnection obtained by the New Vacuum Solar Telescope (NVST) and the Solar Dynamic ...
Zhike Xue   +5 more
openaire   +1 more source

Does Magnetic Reconnection Occur in the Near Lunar Surface Environment?

open access: yesGeophysical Research Letters, 2023
The near lunar surface contains small‐scale magnetic field structures that provide a natural test bed for observing plasmas with a non‐zero Hall electric field, as well as potentially facilitating electron‐only reconnection.
R. P. Sawyer   +7 more
doaj   +1 more source

Solar Flares as Cascades of Reconnecting Magnetic Loops [PDF]

open access: yesPhysical Review Letters, 2003
A model for the solar coronal magnetic field is proposed where multiple directed loops evolve in space and time. Loops injected at small scales are anchored by footpoints of opposite polarity moving randomly on a surface. Nearby footpoints of the same polarity aggregate, and loops can reconnect when they collide.
Hughes, D.   +4 more
openaire   +3 more sources

Experimental Observation Of Energetic Ions Accelerated By Three-Dimensional Magnetic Reconnection In A Laboratory Plasma [PDF]

open access: yes, 2002
Magnetic reconnection is widely believed responsible for heating the solar corona as well as for generating X-rays and energetic particles in solar flares. On astrophysical scales, reconnection in the intergalactic plasma is a prime candidate for a local
Brown, Michael R.   +4 more
core   +3 more sources

Laboratory observation of plasmoid-dominated magnetic reconnection in hybrid collisional-collisionless regime

open access: yesCommunications Physics, 2022
Magnetic reconnection drives the ejection of plasmas during solar flares through changes in the magnetic fields. Here, the authors use a laboratory-based experiment to create magnetic reconnection in a regime in which the plasma on one side of the ...
Zhonghai Zhao   +17 more
doaj   +1 more source

The role of magnetic reconnection in solar activity [PDF]

open access: yes, 1999
We argue that magnetic reconnection plays the determining role in many of the various manifestations of solar activity. In particular, it is the trigger mechanism for the most energetic of solar events, coronal mass ejections and eruptive flares. We propose that in order to obtain explosive eruptions, magnetic reconnection in the corona must have an ...
Antiochos, Spiro K., DeVore, C. Richard
openaire   +4 more sources

Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere

open access: yesThe Astrophysical Journal Letters, 2023
Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause.
M. Nakanotani, G. P. Zank, L.-L. Zhao
doaj   +1 more source

Solar-Type Magnetic Reconnection Model for Magnetar Giant Flares [PDF]

open access: yesPublications of the Astronomical Society of Japan, 2008
Abstract We present a theoretical model describing magnetar giant flares on the basis of solar flare/coronal mass ejection theory. In our model, preflare activity plays a crucial role in driving evaporating flows and supplying baryonic matter to the magnetosphere.
Masada, Youhei   +3 more
openaire   +3 more sources

Kinetic Features of Alpha Particles in a Pestchek-like Magnetic Reconnection Event in the Solar Wind Observed by Solar Orbiter

open access: yesThe Astrophysical Journal Letters, 2023
The acceleration and heating of solar wind particles by magnetic reconnection are important mechanisms in space physics. Although alpha particles ( ^4 He ^2+ ) are the second most abundant population of solar wind ions, their kinetic behavior in solar ...
Die Duan   +12 more
doaj   +1 more source

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