The solar cycle variation of coronal mass ejections and the solar wind mass flux

1994 ◽  
Vol 99 (A3) ◽  
pp. 4201 ◽  
Author(s):  
David F. Webb ◽  
Russell A. Howard
2018 ◽  
Vol 13 (S340) ◽  
pp. 175-176 ◽  
Author(s):  
Wageesh Mishra ◽  
Nandita Srivastava ◽  
Zavkiddin Mirtoshev ◽  
Yuming Wang

AbstractCoronal Mass Ejections (CMEs) contribute to the perturbation of solar wind in the heliosphere. Thus, depending on the different phases of the solar cycle and the rate of CME occurrence, contribution of CMEs to solar wind parameters near the Earth changes. In the present study, we examine the long term occurrence rate of CMEs, their speeds, angular widths and masses. We attempt to find correlation between near sun parameters of the CMEs with near the Earth measurements. Importantly, we attempt to find what fraction of the averaged solar wind mass near the Earth is provided by the CMEs during different phases of the solar cycles.


2000 ◽  
Vol 27 (23) ◽  
pp. 3761-3764 ◽  
Author(s):  
I. G. Richardson ◽  
D. Berdichevsky ◽  
M. D. Desch ◽  
C. J. Farrugia

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