Results 101 to 110 of about 48,383 (235)

Determining the Magnetopause Location With SMILE‐SXI Using a Constrained Solar Wind Independent SWCX Model

Journal of Geophysical Research: Space Physics, Volume 131, Issue 1, January 2026.
Abstract The soft X‐ray imager (SXI) on the SMILE mission promises to revolutionize our understanding of the magnetopause by observing solar wind charge exchange emission from the magnetosheath on a global scale. The primary goal of this instrument is to infer the position and shape of the magnetopause from these images.
S. J. Wharton, J. A. Carter, S. Sembay, A. Paganini, V. Maddi, C. Pagani, Z. Clare, A. Samsonov   +7 more
wiley   +1 more source

Basic Pattern of Three-dimensional Magnetic Reconnection within Strongly Turbulent Current Sheets

The Astrophysical Journal
Magnetic reconnection is a fundamental mechanism of driving eruptive phenomena of different scales and may be coupled with turbulence as suggested by recent remote-sensing and in situ observations.
Yulei Wang, Xin Cheng, Mingde Ding
doaj   +1 more source

Magnetic Reconnection in Turbulent Plasmas and Gamma Ray Bursts

, 2012
We discuss how the model of magnetic reconnection in the presence of turbulence proposed inLazarian & Vishniac 1999 makes the reconnection rate independent either of resistivity or microscopic plasma effects, but determined entirely by the magnetic field
Lazarian, A., Yan, Huirong
core   +1 more source

Chromospheric Magnetic Reconnection and Its Possible Relationship to Coronal Heating [PDF]

, 1999
P. A. Sturrock
openalex   +1 more source

Freshly Generated Super Sunrise Plasma Bubbles During the Geomagnetic Storm on November 5–6, 2023

Space Weather, Volume 24, Issue 1, January 2026.
Abstract During the geomagnetic storm on November 5–6, 2023, freshly generated super sunrise equatorial plasma bubbles (EPBs) and associated irregularities over the 80°–140°E sector were observed combining ground‐based and space observations from GNSS, ionosondes, HF Doppler records, and several satellite missions (COSMIC2, Swarm, and DMSP).
Ke Li, Donghe Zhang, Yaoyu Tian, Yi Zeng, Guanglin Yang, Xiukuan Zhao, Guozhu Li, Yongqiang Hao   +7 more
wiley   +1 more source

Predicting Dual‐Satellite Ionospheric Radial Currents From Single‐Satellite Observations With a BiLSTM Model

Space Weather, Volume 24, Issue 1, January 2026.
Abstract Ionospheric radial currents (IRC) can be derived using two methodologies: (a) the single‐satellite approach: Single‐IRC is deduced from magnetic field data of a single satellite (Swarm‐A); (b) the dual‐satellite approach: Dual‐IRC is calculated by coordinated magnetic field measurements of a pair of satellites (Swarm‐A and ‐C).
Hao Xia, Hui Wang, Kedeng Zhang, Ming Wang   +3 more
wiley   +1 more source

Generalised models for torsional spine and fan magnetic reconnection

, 2011
Three-dimensional null points are present in abundance in the solar corona, and the same is likely to be true in other astrophysical environments.
A. K. Al-Hachami, Al-Hachami, D. I. Pontin, Galsgaard, Gray, Hesse, Hornig, K. Galsgaard, Longcope, Luoni, Lynch, Masson, McLaughlin, Pariat, Parnell, Pontin, Pontin, Pontin, Pontin, Pontin, Priest, Rickard, Santos, Schindler, Török, Wyper, Xiao   +26 more
core   +2 more sources

Dipolarization Regions in Mercury's Magnetosphere: Observation of Flux Pileup and Formation of a Substorm Current Wedge

Geophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract At the end of its mission, the MESSENGER spacecraft's orbit intersected Mercury's nightside magnetic equator at low altitudes below 420 km, enabling the first in situ observations of this region, where the magnetic field strength is typically sub‐dipolar.
A. T. Cushen, W. Sun, J. Slavin, R. Dewey, X. Jia, J. Zhao   +5 more
wiley   +1 more source

Numerical Simulation of Oscillatory Magnetic Reconnection Modulated by Solar Convective Motions

The Astrophysical Journal
Oscillatory magnetic reconnection is a periodic magnetic reconnection process, during which the current sheet’s orientation and the magnetic connections change periodically.
Yifu Wang, Lei Ni, Guanchong Cheng, Jialiang Hu, Yuhao Chen, Abdullah Zafar   +5 more
doaj   +1 more source

Cold ions of ionospheric origin observed at the dayside magnetopause and their effects on magnetic reconnection [PDF]

, 2015
Thesis (Ph.D.) University of Alaska Fairbanks, 2015Magnetic reconnection at the dayside magnetopause is one of the most important mechanisms that efficiently transfers solar wind particles, momentum, and energy into the magnetosphere.
Lee, Sun-Hee, 이, 선희
core