Results 121 to 130 of about 49,445 (284)
Space Weather, Volume 23, Issue 8, August 2025.Abstract Forecasting coronal mass ejections (CMEs) remains a challenge, and no reliable, accurate forecasting method has yet been developed. Knowing that CMEs can occur in association with flares, we compare two approaches: (a) forecasting CMEs by coupling to flare forecasting, and (b) forecasting CMEs independently of flare occurrence.
Julio Hernandez Camero, Lucie M. Green
wiley +1 more source
Identifying Coronal Mass Ejection Active Region Sources: An Automated Approach
The Astrophysical JournalIdentifying the source regions of coronal mass ejections (CMEs) is crucial for understanding their origins and improving space weather forecasting. We present an automated algorithm for matching CMEs detected by the Large Angle Spectrometric Coronagraph ...
Julio Hernandez Camero +2 more
doaj +1 more source
Orthopaedic Surgery, Volume 17, Issue 8, Page 2313-2320, August 2025.Modular femoral stem with a skipping size caused serious complications such as distal femoral fractures in Chinese high‐riding DDH patients. A 1 mm increment of the femoral stem is necessary. ABSTRACT Background S‐ROM prosthesis, one well‐used femoral prosthesis in the patients with developmental dysplasia of the hip (DDH), has a skipping size of the ...
Jiafeng Yi +5 more
wiley +1 more source
The Astrophysical JournalThe main driver of the acceleration of solar energetic particles (SEPs) is believed to be shocks driven by coronal mass ejections. Extreme-ultraviolet (EUV) waves are thought to be the propagating footprint of the shock on the solar surface.
Bin Zhuang +7 more
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Journal of Space Weather and Space ClimateThe shape and dynamics of coronal mass ejections (CMEs) vary significantly based on the instrument and wavelength used. This has led to significant debate about the proper definitions of CME/shock fronts, pile-up/compression regions, and core ...
Stepanyuk Oleg, Kozarev Kamen
doaj +1 more source
Slow Solar Wind: Origin in an Independent Small‐Scale Solar Dynamo
Geophysical Research Letters, Volume 52, Issue 13, 16 July 2025.Abstract Separation of the solar wind (SW) into three flow types (coronal mass ejections (CMEs), high speed streams (HSSs), and slow solar wind (SSW)) reveals an inverse relationship between the percentage of time Earth spends in SSW during a year and its annually averaged magnetic field strength (B).
E. W. Cliver +2 more
wiley +1 more source
Solar Mass Ejections and Coronal Holes [PDF]
International Astronomical Union Colloquium, 1996 AbstractIn this paper we present observations of two types of solar mass ejections, which seem to be associated with the location of coronal holes. In the first type, a filament eruption was observed near a coronal hole, which gave rise to a strong interplanetary scintillations, as detected by IPS observations.
openaire +3 more sources
Wind‐Ulysses source location of radio emissions associated with the January 1997 coronal mass ejection [PDF]
, 1998 S. Hoang +4 more
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Interaction between a Coronal Mass Ejection and Comet 67P/Churyumov–Gerasimenko
The Astrophysical JournalThe interaction between a coronal mass ejection (CME) and a comet has been observed several times by in situ observations from the Rosetta Plasma Consortium, which is designed to investigate the cometary magnetosphere of comet 67P/Churyumov–Gerasimenko ...
Zhenguang Huang +8 more
doaj +1 more source
Distortion of the interplanetary magnetic field by three‐dimensional propagation of coronal mass ejections in a structured solar wind [PDF]
, 1999 D. Odstrčil, V. J. Pizzo
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