Solar and interplanetary activities of isolated and non-isolated coronal mass ejections

We report our results on comparison of two halo Coronal Mass Ejections (CME) associated with X-class flares of similar strength (X1.4) but quite different in CME speed and acceleration, similar geo-effectiveness but quite different in Solar Energetic Particle (SEP) intensity. CME1 (non-isolated) was...

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Veröffentlicht in:	Indian journal of physics 2017-07, Vol.91 (7), p.711-720
Hauptverfasser:	Bendict Lawrance, M., Shanmugaraju, A., Moon, Y.-J., Umapathy, S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Astrophysics and Astroparticles Bursting Bursts Corona Coronal mass ejection Geomagnetism Magnetic storms Original Paper Physics Physics and Astronomy Solar corona Solar flares Solar magnetic field Solar physics Strength Sun Time lag
Online-Zugang:	Volltext
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