Results 91 to 100 of about 1,753 (184)
Studies for inferring the global characteristics of coronal mass ejections (CMEs) from multipoint local in situ observations have been undertaken previously, but limited studies have utilized measurements from multiple spacecraft with sufficiently small ...
Anjali Agarwal, Wageesh Mishra
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Ultra‐Low‐L Sub‐MeV Electron Microbursts During the May 2024 Super Storm
Abstract During the May 2024 super storm, we identified sub‐second microburst‐type relativistic electron precipitation events at McIlwain's L∼2 $L\sim 2$ in low‐Earth orbit using the Gamma‐ray Burst Monitor (CGBM) onboard the CALorimetric Electron Telescope on the International Space Station.
Miki Kurihara +16 more
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In past studies, we classified the near-Earth solar wind into three basic flow types based on inspection of solar wind plasma and magnetic field parameters in the OMNI database and additional data (e.g., geomagnetic indices, energetic particle, and ...
Richardson Ian G., Cane Hilary V.
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Detecting Stellar Coronal Mass Ejections via Coronal Dimming in the Extreme Ultraviolet
Stellar flares and coronal mass ejections (CMEs) can strip planetary atmospheres, reducing the potential habitability of terrestrial planets. While flares have been observed for decades, stellar CMEs remain elusive.
James Paul Mason +4 more
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Stellar eruptive events, such as flares and coronal mass ejections (CMEs), can affect planetary habitability by disturbing the stability of their atmospheres.
Nuri Park +2 more
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Intelligent prediction model for geoeffectiveness of coronal mass ejections
Predicting the geoeffectiveness of coronal mass ejections (CMEs) is a core issue in operational space weather forecasting. In recent years, deep learning methods have been increasingly applied to CME geoeffectiveness prediction. However, existing studies
Xin Tang +3 more
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Probing Trails of Coronal Mass Ejections near the Sun
Coronal mass ejections (CMEs) are surrounded by outflows and trailed by rays. These rays are thought to arise from plasmas around CME downstream current sheets, and they can extend beyond 18 solar radii in some cases.
Carlos R. Braga +3 more
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Aims. This study quantifies how uncertainty in physically meaningful coronal mass ejection (CME) and solar-wind inputs propagates into forecast-relevant diagnostics from eruption through heliospheric evolution.
Stamkos S. +3 more
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MHD Forecasting of Solar Wind With Coronal Mass Ejections
We present a model, implemented as an online service, for predicting the speed and density of solar wind in the inner heliosphere and near Earth. The model is based on a numerical magnetohydrodynamics code PLUTO.
S. Arutyunyan +3 more
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Coronal mass ejections and their sheath regions in interplanetary space. [PDF]
Kilpua E, Koskinen HEJ, Pulkkinen TI.
europepmc +1 more source

