Results 11 to 20 of about 23,617 (267)
Magnetic Reconnection Rate in the M6.5 Solar Flare on 2015 June 22
The Astrophysical Journal, 2023 Magnetic reconnection is regarded as the mechanism for the rapid release of magnetic energy stored in active regions during solar flares, and quantitative measurements of the magnetic reconnection rate are essential for understanding solar flares. In the
Bryce Cannon +6 more
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Observation of the Hall Magnetic Reconnection As Close As 56 Solar Radii from the Sun
The Astrophysical Journal, 2023 A few thin current layers were detected in the rear boundary of an interplanetary coronal mass ejection (ICME) observed at 56 solar radii from the Sun as the Parker Solar Probe spacecraft approached the perihelion for the first time, and were caused by ...
Rongsheng Wang +4 more
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The Astrophysical Journal, 2023 Although magnetic reconnection plays a key role in the formation of a solar filament, the detailed formation process is still ambiguous. Combining the observational data from the New Vacuum Solar Telescope and the Solar Dynamics Observatory, we analyzed ...
Liping Yang +9 more
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Differences in the response to CME and CIR drivers of geomagnetic disturbances
Solar-Terrestrial Physics, 2023 Utilizing 1-minute resolution data on the geomagnetic indices SYM-H, AE, solar wind parameters (velocity Vsw and density Np), and z-component Bz of the interplanetary magnetic field (IMF) during solar cycles 23 and 24, we have statistically analyzed the ...
Namuun B. +3 more
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Dimensionality of solar magnetic reconnection
Reviews of Modern Plasma Physics, 2022 AbstractSolar flares are the best examples of astrophysical magnetic reconnection in which the reconnection structure can be studied in detail. The structure is manifested through flare ribbons, intense optical and EUV emissions in footpoints of field lines attached to the coronal reconnection region.
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A solar filament disconnected by magnetic reconnection [PDF]
Astronomy & 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
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Does Magnetic Reconnection Occur in the Near Lunar Surface Environment?
Geophysical 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
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Experimental Observation Of Energetic Ions Accelerated By Three-Dimensional Magnetic Reconnection In A Laboratory Plasma [PDF]
, 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
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Solar Flares as Cascades of Reconnecting Magnetic Loops [PDF]
Physical 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
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Communications 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
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