Results 21 to 30 of about 15,246 (211)
Deflection of Coronal Mass Ejections in Unipolar Ambient Magnetic Fields
The Astrophysical Journal, 2023 The trajectories of coronal mass ejections (CMEs) are often seen to deviate substantially from a purely radial propagation direction. Such deviations occur predominantly in the corona and have been attributed to “channeling” or deflection of the eruptive
Michal Ben-Nun +7 more
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The Astrophysical Journal, 2023 A fundamental property of coronal mass ejections (CMEs) is their radial expansion, which determines the increase in the CME radial size and the decrease in the CME magnetic field strength as the CME propagates.
Bin Zhuang +6 more
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A SOLAR CORONAL JET EVENT TRIGGERS A CORONAL MASS EJECTION [PDF]
The Astrophysical Journal, 2015 We present the multi-point and multi-wavelength observation and analysis on a solar coronal jet and coronal mass ejection (CME) event in this paper. Employing the GCS model, we obtained the real (three-dimensional) heliocentric distance and direction of the CME and found it propagate in a high speed over 1000 km/s .
Jiajia Liu +5 more
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A census of coronal mass ejections on solar-like stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT Coronal mass ejections (CMEs) may have major importance for planetary and stellar evolution. Stellar CME parameters, such as mass and velocity, have yet not been determined statistically. So far only a handful of stellar CMEs has been detected mainly on dMe stars using spectroscopic observations.
H Lammer +10 more
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The Astrophysical Journal, 2023 Two major solar eruptions on AR 12673 produced a Forbush decrease (FD) event (reduction of cosmic rays) on 2017 September 8 and ground-level enhancement (GLE; enhancement of cosmic rays) on 2017 September 10.
Xiao Xia Yu +5 more
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MHD waves at a spherical interface modelling coronal global EIT waves [PDF]
, 2007 Energetically eruptive events such as flares and coronal mass ejections (CMEs) are known to generate global waves, propagating over large distances, sometimes comparable to the solar radius.
Douglas, M., Ballai, I.
core +3 more sources
High Power Laser Science and Engineering, 2013 The driving mechanism of solar flares and coronal mass ejections is a topic of ongoing debate, apart from the consensus that magnetic reconnection plays a key role during the impulsive process.
Quanli Dong +22 more
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Unraveling the Thermodynamic Enigma between Fast and Slow Coronal Mass Ejections
The Astrophysical Journal, 2023 Coronal mass ejections (CMEs) are the most energetic expulsions of magnetized plasma from the Sun that play a crucial role in space weather dynamics.
Soumyaranjan Khuntia +5 more
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A Model for Solar Coronal Mass Ejections [PDF]
The Astrophysical Journal, 1999 Astrophysical Journal latex file, 28 pages, 8 color and 2 b-w figures (gif files)
Antiochos, S. K. +2 more
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Frontiers in Astronomy and Space Sciences, 2023 Solar coronal jets are frequently occurring collimated ejections of solar plasma, originating from magnetically mixed polarity locations on the Sun of size scale comparable to that of a supergranule.
Alphonse C. Sterling +8 more
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