2 papers
astro-ph.SR2024
Origins of Very Low Helium Abundance Streams Detected in the Solar Wind Plasma
Yogesh, N. Gopalswamy, D. Chakrabarty +4
The abundance of helium () in the solar wind exhibits variations typically in the range from 2-5% with respect to solar cycle activity and solar wind velocity. However, the…
astro-ph.SR2018
Solar cycle variation of coronal mass ejections contribution to solar wind mass flux
Wageesh Mishra, Nandita Srivastava, Zavkiddin Mirtoshev +1
Coronal Mass Ejections (CMEs) contributes to the perturbation of solar wind in the heliosphere. Thus, depending on the different phases of the solar cycle and the rate of CME occur…