activity
20152019
most citedMass Loss via Solar Wind and Coronal Mass Ejections During Solar Cycle 23 and 24

32 citations · 82 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2022

Evolution and Consequences of Coronal Mass Ejections in the Heliosphere

Wageesh Mishra

Investigating the heliospheric evolution and consequences of Coronal mass ejections (CMEs) is critical to understanding the solar-terrestrial relationship. For the first time, Heli…

astro-ph.SR201932 cited

Mass Loss via Solar Wind and Coronal Mass Ejections During Solar Cycle 23 and 24

Wageesh Mishra, Nandita Srivastava, Yuming Wang +3

Similar to the Sun, other stars shed mass and magnetic flux via ubiquitous quasi-steady wind and episodic stellar coronal mass ejections (CMEs). We investigate the mass loss rate v…

physics.space-ph2018

Torsional Alfven wave embedded ICME magnetic cloud and corresponding geomagnetic storm

Anil N. Raghav, Ankita Kule, Ankush Bhaskar +3

The energy transfer during the interaction of large-scale solar wind structure and the Earth's magnetosphere is the chronic issue in space-weather studies. To understand this, rese…

astro-ph.SR2018

Modeling the thermodynamic evolution of Coronal Mass Ejections (CMEs) using their kinematics

Wageesh Mishra, Yuming Wang

Earlier studies on Coronal Mass Ejections (CMEs), using remote sensing and in situ observations, have attempted to determine some of the internal properties of CMEs, which were lim…

astro-ph.SR2018

Study of Interplanetary and Geomagnetic Response of Filament Associated CMEs

Kunjal Dave, Wageesh Mishra, Nandita Srivastava +1

It has been established that Coronal Mass Ejections (CMEs) may have significant impact on terrestrial magnetic field and lead to space weather events. In the present study, we sele…

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…