Results 131 to 140 of about 23,617 (267)
Key issues on magnetic reconnection at Mercury
Magnetic reconnection processes and their impact on planetary magnetospheric dynamics exhibit significant differences due to differences in upstream solar wind conditions and internal planetary environments.
Jun Zhong
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OBSERVATION OF MAGNETIC RECONNECTION AT A 3D NULL POINT ASSOCIATED WITH A SOLAR ERUPTION [PDF]
J. Q. Sun +4 more
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Alfvén Waves from Interchange Reconnection at Separators as a Possible Source of Switchbacks
Parker Solar Probe has observed Alfvénic fluctuations of amplitude large enough to occasionally reverse the local magnetic field direction—a phenomenon known as a switchback. Some have attributed switchbacks to reconnection in the low corona between open
Dana Longcope, Philip Klaassen
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SLIPPING MAGNETIC RECONNECTION, CHROMOSPHERIC EVAPORATION, IMPLOSION, AND PRECURSORS IN THE 2014 SEPTEMBER 10 X1.6-CLASS SOLAR FLARE [PDF]
Jaroslav Dudík +9 more
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Failure of a Solar Filament Eruption Caused by Magnetic Reconnection with Overlying Coronal Loops [PDF]
Leping Li +13 more
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Magnetic reconnection and particle acceleration in the solar wind: theory, observations and opinions
Olga Khabarova
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Magnetic reconnection and the Kelvin-Helmholtz instability in the solar\n corona [PDF]
T. A. Howson +2 more
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Active region NOAA 13842 produced two successive solar flares: an X7.1-class flare on 2024 October 1, and an X9.0-class flare on 2024 October 3. This study continues our previous simulation work that successfully reproduced the X7.1-class solar flare. In
Keitarou Matsumoto +7 more
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Spontaneous non-steady magnetic reconnection within the solar environment [PDF]
Lapo Bettarini, Giovanni Lapenta
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