RESEARCH INTEREST

My research work is focused on the magnetic reconnection, MHD instabilities in the solar eruptions and their consequences on space weather. My aim is to form a bridge between the observational aspect of magnetic reconnection, solar eruptions, and MHD plasma processes with the theoretical understanding.

Internal Dynamics of Solar Prominence/Filaments

• I am exploring the internal dynamics of solar prominences in terms of different types of instabilities and reconnection. Using multi-wavelength imaging, spectroscopic, and stereoscopic observations, I am also study the role of the internal dynamics to initiate or de-stabilized the prominence/filament eruptions, its thermal behavior scenarios and how these internal dynamics scenarios can be use as a tool to govern the seismology of the filaments/prominence.

Evolution of Instability in Different Solar Structures

• Using multi-wavelength solar imaging observations, I worked on the evolution of different-types of instabilities in different magnetized structures (e.g., prominence/filaments, jets, loops, etc.) of the solar atmosphere.

Magnetic Reconnection

• I worked on the different aspects of magnetic reconnection, forced reconnection, its role to initiate the small to large-scale solar eruptions, and its contribution in the coronal heating.

Coronal Mass Ejections (CMEs) and Space Weather

• I also worked on the initiation process of CMEs, its propagation in the interplanetary space, and their impact on the Earth's space weather.