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Published in 2021 at "Astronomische Nachrichten"
DOI: 10.1002/asna.20210100
Abstract: Present Address Leibniz Institute for Astrophysics (AIP) An der Sternwarte 16, 14482 Potsdam, Germany Coronal mass ejections (CMEs) are more energetic than any other class of solar phenomena. They arise from the rapid release of…
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Keywords:
numerical perspective;
ejections exoplanets;
mass;
exoplanets numerical ... See more keywords
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Published in 2017 at "Solar Physics"
DOI: 10.1007/s11207-017-1129-9
Abstract: Observational and numerical studies have shown that the kinematic characteristics of two or more coronal mass ejections (CMEs) may change significantly after a CME collision. The collision of CMEs can have a different nature, i.e.…
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Keywords:
definition;
two coronal;
collision;
mass ejections ... See more keywords
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Published in 2020 at "Solar Physics"
DOI: 10.1007/s11207-020-01721-0
Abstract: Interplanetary coronal mass ejections (ICMEs) primarily move radially as they propagate away from the Sun, maintaining approximately constant angular width with respect to the Sun. As ICMEs have typical angular widths of around $60^{\circ }$…
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Keywords:
coherence coronal;
coherence;
mass ejections;
magnetic clouds ... See more keywords
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Published in 2019 at "Journal of Astrophysics and Astronomy"
DOI: 10.1007/s12036-018-9570-1
Abstract: Solar flares and coronal mass ejections (CMEs) are two very important active events from Sun. Inspite of several theoretical and statistical analyses, the relation between solar flares and CMEs is so far not well established,…
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Keywords:
coronal mass;
mass ejections;
solar flares;
relation solar ... See more keywords
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Published in 2018 at "Planetary and Space Science"
DOI: 10.1016/j.pss.2018.01.012
Abstract: Abstract A coronal mass ejections (CME) is the huge mass of plasma with embedded magnetic field ejected abruptly from the Sun. These CMEs propagate into interplanetary space with different speed. Some of them hit the…
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Keywords:
earth magnetosphere;
mass;
geomagnetic response;
mass ejections ... See more keywords
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Published in 2020 at "Space Weather"
DOI: 10.1029/2019sw002246
Abstract: Predictions of the impact of coronal mass ejections (CMEs) in the heliosphere mostly rely on cone CME models, whose performances are optimized for locations in the ecliptic plane and at 1 AU (e.g., at Earth).…
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Keywords:
coronal mass;
mass ejections;
cone;
cmes using ... See more keywords
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Published in 2017 at "Nature"
DOI: 10.1038/nature22050
Abstract: Magnetically driven eruptions on the Sun, from stellar-scale coronal mass ejections to small-scale coronal X-ray and extreme-ultraviolet jets, have frequently been observed to involve the ejection of the highly stressed magnetic flux of a filament.…
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Keywords:
solar eruptions;
universal model;
mass;
model solar ... See more keywords
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Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/201936016
Abstract: Our aim is to investigate the possible physical association between consecutive coronal mass ejections (CMEs). Through a statistical study of the main characteristics of 27761 CMEs observed by SOHO/LASCO during the past 20 years. We…
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Keywords:
space time;
time;
association;
mass ejections ... See more keywords
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Published in 2017 at "Physics of Plasmas"
DOI: 10.1063/1.4993929
Abstract: Solar eruptions, observed as flares and coronal mass ejections (CMEs), are the most energetic visible plasma phenomena in the solar system. CMEs are the central component of solar eruptions and are detected as coherent magnetized…
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Keywords:
physics erupting;
coronal mass;
physics;
ejections cmes ... See more keywords
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Published in 2017 at "Geomagnetism and Aeronomy"
DOI: 10.1134/s0016793217070258
Abstract: The observed variations of the magnetic properties of sunspots during eruptive events (solar flares and coronal mass ejections (CMEs)) are discussed. Variations of the magnetic field characteristics in the umbra of the sunspots of active…
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Keywords:
flares coronal;
field;
field characteristics;
mass ejections ... See more keywords
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Published in 2018 at "Physics of Atomic Nuclei"
DOI: 10.1134/s106377881809003x
Abstract: Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is…
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Keywords:
muon flux;
studying anisotropy;
coronal mass;
mass ejections ... See more keywords