Results 91 to 100 of about 2,611,112 (157)
Magnetic reconnection is an important physical process of energy conversion in the heliosphere. Parker Solar Probe (PSP) passes through current sheets of the inner heliosphere and is likely to encounter magnetic reconnection events there. PSP traversed a
Rui Zhuo +4 more
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Magnetic reconnection drives a wide range of astrophysical phenomena, including geomagnetic storms, solar flares, and activity in blazars. However, direct measurement of key reconnection observables remains challenging due to the remote and extreme ...
Sergey K. Ermakov +6 more
doaj +1 more source
Formation of Fan-spine Magnetic Topology through Flux Emergence and Subsequent Jet Production
Fan-spine magnetic structure, as a fundamental three-dimensional topology in magnetic reconnection theory, plays a crucial role in producing solar jets. However, how fan-spine configurations form in the solar atmosphere remains elusive. Using the Chinese
Yadan Duan +6 more
doaj +1 more source
The extreme solar storm of 2024 May 10, during the 25th solar cycle, which recorded a symmetric H component index (Sym-H) reaching −500 nT, was the strongest since the 2003 Halloween storm.
Shibotosh Biswas +6 more
doaj +1 more source
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
doaj +1 more source
In situ observations by Parker Solar Probe (PSP) suggest that the heliospheric current sheet (HCS) undergoes near-continuous magnetic reconnection close to the Sun, in stark contrast to scarce observations of this phenomenon in the HCS at 1 au.
Harry C. Lewis +10 more
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Kinetic Simulation of Energy Cascade Associated with Filamentary Currents in Solar Wind Turbulence
The role of magnetic reconnection in energy cascade within solar wind turbulence remains a fundamental unsolved problem in astrophysics. We employ a coarse-grained technique to investigate energy cascades at sub-ion scale within filamentary currents (FCs)
Meng Zhang +6 more
doaj +1 more source
Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions. [PDF]
Cairns IH +41 more
europepmc +1 more source
Potential Solar Precursors to Magnetic Switchbacks. [PDF]
Tripathi D +11 more
europepmc +1 more source
Propagating slow-mode shocks discovered in dynamical solar flare loops. [PDF]
Ye J +8 more
europepmc +1 more source

