Results 131 to 140 of about 22,968 (238)
Abstract The CLEAR Space Weather Center of Excellence's solar energetic particle (SEP) model, SOlar wind with FIeld lines and Energetic particles (SOFIE), was run and evaluated on‐site during the Space Weather Prediction Testbed (SWPT) exercise at the National Oceanic and Atmospheric Administration's Space Weather Prediction Center (NOAA/SWPC) in May ...
Weihao Liu +31 more
wiley +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
Abstract We studied the characteristics of ultra‐low‐frequency (ULF) waves associated with dipolarization in the near‐Earth plasma sheet for substorms and pseudosubstorms, employing superposed epoch analysis of data from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft.
Kanpatom Kasonsuwan +2 more
wiley +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
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
doaj +1 more source
Abstract Substorms are often described by a loading‐unloading cycle, where onset follows gradual accumulation of solar wind magnetic flux in the magnetosphere. Yet observations indicate that intense substorms can also be directly driven, though the underlying mechanism remains unresolved.
Yong Ren +8 more
wiley +1 more source
Spectral Properties and Energy Injection in Mercury's Magnetotail Current Sheet
Abstract Mercury's magnetotail hosts a thin and highly dynamic current sheet (CS), where magnetic reconnection and strong fluctuations frequently occur. Here, we statistically analyze magnetic field power spectra across 370 magnetotail CSs observed by MESSENGER.
Xinmin Li +10 more
wiley +1 more source
Abstract Due to the lack of low‐altitude (<∼ ${< } \sim $50 km), high‐time‐resolution measurements, expected electron‐only magnetic reconnection near lunar magnetic anomalies (LMAs) has not been directly observed by lunar orbiters even though it is expected from numerical simulations and laboratory experiments.
Kohei Ogino +8 more
wiley +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
Current sheet formation and magnetic reconnection in solar magnetic fields
Diese Arbeit beschreibt magnetische Rekonnexion an dünnen Stromschichten in Konfigurationen ohne verschwindendes Magnetfeld. Dabei wird eine Methode entwickelt, die die Bestimmung der Rekonnexionsrate ohne die Einbeziehung eines parallelen elektrischen Feldes ermöglicht. Zusätzlich werden grundsätzliche geometrische Unterschiede zwischen Rekonnexion in
openaire +3 more sources

