I am a a postdoctoral fellow under CEFIPRA at IUCAA working on the topic of Investigation of the Origin of Switchbacks in the Solar Corona via Interchange Reconnection: A Statistical and Multi-instruments Approach Including Machine Learning. My academic interests include solar physics, stellar physics, main sequence stars, radiative transfer for 1D and 3D atmospheric models, in-situ, optical and radio observations, in general, computational solar-stellar astrophysics. And you can read about my interests and struggles here. I also like to share my science with everyone, by writing articles, giving talks, or just any way possible!
I conducted my PhD research in the EMISSA project at RoCS at the Institute of Theoretical Astrophysics at the University of Oslo, Norway. The thesis titled 'A new look at Solar-Stellar Activity with the Atacama Large Millimeter/submillimeter Array', explores the Sun as a benchmark for studying sun-like stars, employing spectral lines like Ca II and Hα to examine their atmospheric activity along with the millimetre data from Atacama Large Millimetre/submillimetre (ALMA), which offers a fresh perspective on stellar activity and thermal structure. Comparing synthetic spectra with millimetre maps and combining long-term solar observations from ALMA with various diagnostic tools reveals thermal structure and long-term variations in the solar activity, which emphasises ALMA's pivotal role in advancing our understanding of solar and stellar activity.
I did my BS-MS Dual Degree in Science with a major in Physics and a minor in Engineering Science in IISER Bhopal with an MS Thesis titled Study of Phase Transitions from Neutron Stars to Quark Stars. My other interests are recreational writing, professional classical dancing, travelling and playing cricket.
I conducted my PhD research in the EMISSA project at RoCS at the Institute of Theoretical Astrophysics at the University of Oslo, Norway. The thesis titled 'A new look at Solar-Stellar Activity with the Atacama Large Millimeter/submillimeter Array', explores the Sun as a benchmark for studying sun-like stars, employing spectral lines like Ca II and Hα to examine their atmospheric activity along with the millimetre data from Atacama Large Millimetre/submillimetre (ALMA), which offers a fresh perspective on stellar activity and thermal structure. Comparing synthetic spectra with millimetre maps and combining long-term solar observations from ALMA with various diagnostic tools reveals thermal structure and long-term variations in the solar activity, which emphasises ALMA's pivotal role in advancing our understanding of solar and stellar activity.
I did my BS-MS Dual Degree in Science with a major in Physics and a minor in Engineering Science in IISER Bhopal with an MS Thesis titled Study of Phase Transitions from Neutron Stars to Quark Stars. My other interests are recreational writing, professional classical dancing, travelling and playing cricket.
