Results 61 to 70 of about 1,576,389 (170)

Impacts of Neutral Wind‐Driven Currents on Geomagnetic Disturbances and Magnetospheric Dynamics During the May 2024 Storm

Journal of Geophysical Research: Space Physics, Volume 131, Issue 9, September 2026.
Abstract The neutral wind dynamo generates ionospheric currents that can significantly affect high‐latitude electrodynamics during geomagnetic storms, yet its role in global magnetosphere‐ionosphere coupling is often underrepresented. We quantify the impact of wind‐driven currents on geomagnetic disturbances (GMDs) and magnetospheric dynamics during ...
Yu Hong, Yue Deng, Cheng Sheng, Daniel Welling, Colin Waters   +4 more
wiley   +1 more source

Simulation of Thermal Nonequilibrium Cycles in the Solar Wind

The Astrophysical Journal
Thermal nonequilibrium (TNE) is a condition of the plasma in the solar corona in which the local rate of energy loss due to radiation increases to the point that it cannot be sustained by the various heating terms acting on the plasma, precluding the ...
Roger B. Scott, Jeffrey W. Reep, Mark G. Linton, Stephen J. Bradshaw   +3 more
doaj   +1 more source

Rapid Magnetotail Reconfiguration and Ion‐Scale Wave Activity at Mercury

Journal of Geophysical Research: Space Physics, Volume 131, Issue 9, September 2026.
Abstract Mercury's magnetosphere is an extremely dynamic environment, where substorm‐like activity, including dipolarization fronts and particle acceleration, periodically disrupts the stability and radial extent of the closed field line region. The common narrowband ∼1 Hz waves at Mercury, near the local proton gyrofrequency are preferentially ...
M. Persson, R. M. Dewey, A. I. Eriksson, M. André, E. Yordanova, L. Richard, A. Dagore, J.‐E. Wahlund   +7 more
wiley   +1 more source

Kinetic Physics of the Solar Corona and Solar Wind

Living Reviews in Solar Physics, 2006
Kinetic plasma physics of the solar corona and solar wind are reviewed with emphasis on the theoretical understanding of the in situ measurements of solar wind particles and waves, as well as on the remote-sensing observations of the solar corona made by
Marsch Eckart
doaj  

Space Weather Mitigation Decisions by Critical Infrastructure Operators During Solar Cycle 25

Space Weather, Volume 24, Issue 9, September 2026.
Abstract The “Gannon Storm” in May 2024 was the largest space weather event experienced in 20 years, generating auroras at latitudes as low as 35°, visible in Florida and Mexico. Such events pose significant operational challenges for critical infrastructure operators, particularly those managing electricity transmission networks, satellite ...
C. M. LaNeve, E. J. Oughton, N. Rivera, R. S. Weigel, D. Thomas, C. T. Gaunt   +5 more
wiley   +1 more source

Coronal Rain Driven by Low-frequency Impulsive Heating: Dependence of Dynamics and Morphology on Coronal Heating and Magnetic Field

The Astrophysical Journal
We performed numerical simulations to investigate how coronal heating and magnetic field strength regulate the dynamics and morphology of coronal rain in the solar corona.
Takero Yoshihisa, Takaaki Yokoyama
doaj   +1 more source

Benchmarking Deep Learning Models for Real‐Time Prediction of Post‐Peak Solar Flare Irradiance Using FISM2 Data

Space Weather, Volume 24, Issue 9, September 2026.
Abstract This study presents a deep learning framework for real‐time prediction of post‐peak solar flare irradiance. The model targets the soft X‐ray band (0.1–0.8 nm) and three extreme ultraviolet (EUV) wavelength bands (9.0–9.9 nm, 13.0–13.9 nm, and 30.0–30.9 nm), and produces forecasts at 1‐min cadence for 3 hr after the flare peak.
Jeong‐Heon Kim, Junmu Youn, Sung‐Hong Park, Seungwoo Ahn, Young‐Sil Kwak, Yong‐Jae Moon, P. C. Chamberlin   +6 more
wiley   +1 more source

Atmospheric Heating Events Associated with Fine-scale Flux Emergence in Ephemeral Regions

The Astrophysical Journal
Coronal heating has puzzled solar physicists for decades. The question of why the Sun’s upper atmosphere is significantly hotter than its lower atmosphere remains a key mystery.
Hanlin Yang, Jingxiu Wang, Chunlan Jin
doaj   +1 more source

Modeling the Propagation of Slow Magnetoacoustic Waves in a Multistranded Coronal Loop

The Astrophysical Journal
We study the propagation properties of slow magnetoacoustic waves in a multithermal coronal loop using a 3D MHD model, for the first time. A bundle of 33 vertical cylinders, each of 100 km radius, randomly distributed over a circular region of radius 1 ...
S. Krishna Prasad, T. Van Doorsselaere
doaj   +1 more source

Coronal heating in multiple magnetic threads [PDF]

, 2015
We acknowledge the financial support of STFC through the Consolidated grant to the University of St Andrews.Context. Heating the solar corona to several million degrees requires the conversion of magnetic energy into thermal energy.
Cargill, Peter, Hood, Alan William, Hood, AW, P. J. Cargill, Cargill, PJ, Browning, Philippa, K. V. Tam, Tam, Kuan Vai, Tam, KV, P. K. Browning, Browning, PK, A. W. Hood, Browning, PK; id_orcid, Tam, [Unknown], Hood, Alan William; id_orcid   +14 more
core   +1 more source