Solar cycle variation of coronal mass ejections contribution to solar wind mass flux
Wageesh MishraUniversity of Science and Technology of China, ChinaNandita SrivastavaUdaipur Solar Observatory, Physical Research Laboratory, Udaipur-313001, IndiaZavkiddin MirtoshevDepartment of Physics, Samarkand State University, Samarkand- 140104, UzbekistanYuming WangUniversity of Science and Technology of China, China
ABI
Abstract
Abstract Coronal 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.
Topics
Identifiers
Citations and references
Cited by 03 references
Metrics — AkademScholar · Coming soon