Results 61 to 70 of about 2,458,506 (201)
Observations of a Quickly Flapping Interplanetary Magnetic Reconnection Exhaust
Frontiers in Physics, 2021 On the basis of the Petschek reconnection model and the characteristics of reconnection, hundreds of reconnection exhausts were reported in the solar wind.
Jiemin Wang +3 more
doaj +1 more source
Controls on Solar Wind Entry Identified Through Wind–ACE Heavy‐Ion Diagnostics
Geophysical Research Letters, Volume 53, Issue 16, 28 August 2026.Abstract Solar wind (SW) entry into the magnetosphere occurs through several mechanisms, but their dependence on the properties of different ion species is unknown. We compare measurements from Wind‐STICS (magnetosphere) with ACE‐SWICS (L1) to test for any preferential entry between He2+ and SW heavy ions.
S. Colón‐Rodríguez +3 more
wiley +1 more source
Asymmetric Magnetic Reconnection In The Solar Atmosphere
, 2013 Models of solar flares and coronal mass ejections typically predict the development of an elongated current sheet in the wake behind the rising flux rope. In reality, reconnection in these current sheets will be asymmetric along the inflow, outflow, and out-of-plane directions.
Murphy, Nicholas A. +10 more
openaire +2 more sources
The Astrophysical JournalAlthough multiscale filament eruptions serve as significant triggers for various energetic release processes in the solar atmosphere, the underlying mechanisms remain elusive.
Liping Yang +13 more
doaj +1 more source
The Astrophysical Journal, 2023 Different from the classical emerging-flux model for solar jets, recent studies proposed that the great majority of solar coronal jets are triggered by minifilament eruptions and two magnetic reconnection processes should take place during the course ...
Jiayan Yang +4 more
doaj +1 more source
Variations of Mid‐Magnetotail Magnetic Pressure During Substorms
Geophysical Research Letters, Volume 53, Issue 16, 28 August 2026.Abstract Magnetic reconnection is commonly observed in the mid‐tail plasma sheet during substorms, the mechanism behind this spatial preference, however, remains unsolved. This study focuses on magnetic pressure evolution within this critical region during substorms.
Xiaowei Ma +3 more
wiley +1 more source
Imaging Observations of Magnetic Reconnection in a Solar Eruptive Flare [PDF]
The Astrophysical Journal, 2017 Abstract Solar flares are among the most energetic events in the solar atmosphere. It is widely accepted that flares are powered by magnetic reconnection in the corona. An eruptive flare is usually accompanied by a coronal mass ejection, both of which are probably driven by the eruption of a magnetic flux rope (MFR).
Y. Li +4 more
openaire +4 more sources
The Astrophysical JournalMagnetic reconnection is widely believed to be the fundamental process in the solar atmosphere that underlies magnetic energy release and particle acceleration.
Pankaj Kumar +4 more
doaj +1 more source
Global Plasmaspheric Refilling Rates Inferred From Deep‐Learning Electron Density Reconstructions
Geophysical Research Letters, Volume 53, Issue 16, 28 August 2026.Abstract As a key process in magnetosphere‐ionosphere coupling, plasmaspheric refilling is a long‐standing focus in space physics. In this study, we develop a global electron density (GEO‐NE) model based on a CNN‐Transformer architecture, and use the model to investigate plasmaspheric electron density refilling rates. Using global electron density maps
Zhenyu Guo +6 more
wiley +1 more source
Geophysical Research Letters, 2016 Magnetic reconnection at the Earth's magnetopause is the primary process by which solar wind plasma and energy gains access to the magnetosphere. One indication that magnetic reconnection is occurring is the observation of accelerated plasma as a jet ...
S. M. Petrinec +13 more
doaj +1 more source