Results 181 to 190 of about 54,745 (274)
Turn on the super-elastic collision nature of coronal mass ejections through low approaching speed. [PDF]
Sci Rep, 2016 Shen F, Wang Y, Shen C, Feng X.
europepmc +1 more source
The Sun’s magnetized plasma atmosphere is the source of various forms of activity, the most dramatic of which are coronal mass ejections (CMEs). These ejections are a bulk expulsion of plasma and magnetic field that travel out into the heliosphere ...
Green, Lucie M
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Evolution of interplanetary coronal mass ejections
, 2011 Title: Evolution of Interplanetary Coronal Mass Ejections Author: Andrii Lynnyk Department: Department of Surface and Plasma Science Supervisor: RNDr. Marek Vandas, DrSc.
Lynnyk, Andrii
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Coronal Mass Ejections - A Statistical View
, 2008 Although first recognized in 1971, the quasi-continuous record since 1979 of the appearance of coronal mass ejections (CMEs-perhaps more appropriately called coronal magnetic ejections) has resulted in a stable understanding of their properties, at least
Cremades, H., SaintCyr, O. C.
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On the topology of global coronal magnetic fields
, 2014 This thesis considers the magnetic topology of the global solar corona. To understand the magnetic topology we use the magnetic skeleton which provides us with a robust description of the magnetic field.
Edwards, Sarah J.
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Relationship of interplanetary coronal mass ejections with geomagnetic activity
, 2008 244-248The signatures of Coronal Mass Ejection (CME) associated interplanetary disturbances are called as Interplanetary Coronal Mass Ejections (ICMEs).
Shrivastava, Pankaj K, Singh, Geeta
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, 2013 We have studied statistically correlative analysis of long-term modulation of cosmic ray intensity (CRI) with coronal mass ejections and solar flare index for the period of 1997 to 2010 (23rd and 24th solar cycle).
Patel, Nand Kumar +3 more
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Coronal Mass Ejections and Non-recurrent Forbush Decreases
, 2014 Coronal mass ejections (CMEs) and their interplanetary counterparts (interplanetary coronal mass ejections, ICMEs) are responsible for large solar energetic particle events and severe geomagnetic storms. They can modulate the intensity of Galactic cosmic
Abunina, M. +9 more
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Solwind observations of coronal mass ejections during 1979-1985
, 1986 Coronal observations have been processed for parts of each year during the interval 1979-1985. Around sunspot maximum, coronal mass ejections (CMEs) occurred at the rate of approximately 2 per day, and had a wide range of physical and morphological ...
Howard, R. A. +3 more
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STEREO Observations of Interplanetary Coronal Mass Ejections in 2007–2016
, 2018 L. Jian +3 more
semanticscholar +1 more source