Results 21 to 30 of about 62,110 (306)
Investigating Remote-Sensing Techniques to Reveal Stealth Coronal Mass Ejections
Frontiers in Astronomy and Space Sciences, 2021 Eruptions of coronal mass ejections (CMEs) from the Sun are usually associated with a number of signatures that can be identified in solar disc imagery. However, there are cases in which a CME that is well observed in coronagraph data is missing a clear ...
Erika Palmerio +13 more
doaj +1 more source
Hot prominence detected in the core of a coronal mass ejection [PDF]
Astronomy & Astrophysics, 2018 Context. We study an erupting prominence embedded in the core of a coronal mass ejection that occurred on August 2, 2000, and focus on deriving the plasma filling factor of the prominence. Aims. We explore two methods for measuring this factor along the
R. Susino +3 more
semanticscholar +1 more source
The Drag-based Ensemble Model (DBEM) for Coronal Mass Ejection Propagation [PDF]
, 2018 The drag-based model for heliospheric propagation of coronal mass ejections (CMEs) is a widely used analytical model that can predict CME arrival time and speed at a given heliospheric location.
M. Dumbovi'c +6 more
semanticscholar +1 more source
Forward Modeling of Coronal Mass Ejection Flux Ropes in the Inner Heliosphere with 3DCORE [PDF]
Space weather : the international journal of research & applications, 2017 Forecasting the geomagnetic effects of solar storms, known as coronal mass ejections (CMEs), is currently severely limited by our inability to predict the magnetic field configuration in the CME magnetic core and by observational effects of a single ...
C. Möstl +9 more
semanticscholar +1 more source
Coronal Mass Ejections: Observations [PDF]
Living Reviews in Solar Physics, 2012 Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic particles, and radio bursts. Since the vast majority of these are associated with the eruption, development, and evolution of coronal mass ejections (CMEs), we focus on CME observations in this review. CMEs are a key aspect of coronal and interplanetary dynamics.
David F. Webb, Timothy A. Howard
openaire +3 more sources
COMPOSITION OF CORONAL MASS EJECTIONS [PDF]
The Astrophysical Journal, 2016 ABSTRACT We analyze the physical origin of plasmas that are ejected from the solar corona. To address this issue, we perform a comprehensive analysis of the elemental composition of interplanetary coronal mass ejections (ICMEs) using recently released elemental composition data for Fe, Mg, Si, S, C, N, Ne, and He as compared to O and H ...
Susan T. Lepri +6 more
openaire +4 more sources
On the Construction of Phenomenological Coronal Mass Ejection Models
Space Weather, 2021 We consider recently developed 3DCORE coronal mass ejection (CME) model. We find that the magnetic field of 3DCORE violates both Maxwellian equations: the one for absence of magnetic monopoles and the other one for Faraday induction (“frozen‐in ...
D. V. Peregoudov
doaj +1 more source
Earth-affecting solar transients: a review of progresses in solar cycle 24
Progress in Earth and Planetary Science, 2021 This review article summarizes the advancement in the studies of Earth-affecting solar transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort of the International Study of Earth-affecting Solar Transients (ISEST)
Jie Zhang +18 more
doaj +1 more source
CHROMOSPHERE TO 1 au SIMULATION OF THE 2011 MARCH 7th EVENT: A COMPREHENSIVE STUDY OF CORONAL MASS EJECTION PROPAGATION [PDF]
, 2016 We perform and analyze the results of a global magnetohydrodynamic simulation of the fast coronal mass ejection (CME) that occurred on 2011 March 7. The simulation is made using the newly developed Alfvén Wave Solar Model (AWSoM), which describes the ...
M. Jin +7 more
semanticscholar +1 more source
Flux Accretion and Coronal Mass Ejection Dynamics [PDF]
Solar Physics, 2017 Coronal mass ejections (CMEs) are the primary drivers of severe space weather disturbances in the heliosphere. Models of CME dynamics have been proposed that do not fully include the effects of magnetic reconnection on the forces driving the ejection ...
B. Welsch
semanticscholar +1 more source