Bio: Hi, I am a Postdoctoral Scholar in the Department of Atmospheric and Oceanic Sciences at the University of California, Los Angeles (UCLA).
I received my Ph.D. in Space Physics from the Center of Excellence in Space Sciences India (CESSI), Indian Institute of Science Education and Research (IISER) Kolkata, under the supervision of Prof. Dibyendu Nandi. My doctoral research focused on understanding the interaction of coronal mass ejections with planetary magnetospheres and developing physics-based models to predict their geomagnetic impact.
My research lies within the broader field of solar-terrestrial physics, with interests in heliophysics, space weather, magnetosphere-ionosphere coupling, multi-fluid magnetohydrodynamics (MHD), ionospheric outflow, and plasma sheet dynamics.
As a Scientist and Developer with the NASA DRIVE Science Center for Geospace Storms (CGS), I contribute to the development of the Multiscale Atmosphere-Geospace Environment (MAGE) model. My current work focuses on advancing next-generation global magnetosphere simulations by incorporating multi-fluid physics to investigate ionospheric outflow, heavy-ion transport, plasma sheet composition, and the dynamics of geomagnetic storms.
My research combines high-performance computing, numerical modeling, and satellite observations to improve the physical understanding and prediction of space weather across the coupled Sun-Earth system.
Prior to my doctoral studies, I completed an M.Sc. in Physics from West Bengal State University and a B.Sc. (Honours) in Physics from Rishi Bankim Chandra College. Alongside research, I have served as a teaching assistant, presented my work at numerous international conferences, and contributed to collaborative research within the global heliophysics community.
Beyond research, I enjoy writing Bengali poetry, exploring the world through mobile photography, and sharing the excitement of space science with a broader audience.
Heliophysics and the coupled Sun-Earth system.
Global plasma simulations and high-performance computing.
Physics-based forecasting of geomagnetic disturbances.
Ionospheric outflow, plasma transport, and magnetospheric dynamics.
Heavy-ion transport, composition, and energy evolution.
Solar eruptions, their impact on planetary magnetospheres, Storm-time dynamics, ring current evolution, and geomagnetic activity.
Scientific computing, numerical modeling, and data-driven analysis.
Multi-mission observations and validation of numerical simulations.
Solar wind interaction with the Moon and planetary plasma environments.
Visualization, analysis, and interpretation of large-scale simulation data.
Affiliation: Center of Excellence in Space Sciences India (CESSI), Indian Institute of Science Education and Research (IISER) Kolkata, Mohanpur, India
CGPA (Course Work): 9.38/10.00
Supervisor: Prof. Dibyendu Nandi
Thesis: Modeling the Impact of Space Weather on Planetary Space Environments.
Affiliation: West Bengal State University, Barasat, India
CGPA: 5.13/6.00
Specialization: Astrophysics, Cosmology, Computational Physics, High Energy Physics
MSc Thesis: Accretion properties of rotating naked singularities and the generalised pseudo-Newtonian potential for studying accretion disk dynamics of rotating naked singularities.
Advisor: Prof. Parthasarathi Joarder
Institute: Centre for Astroparticle Physics & Space Sciences, Bose Institute, Kolkata, India
Affiliation: Rishi Bankim Chandra College, Naihati, India
University: West Bengal State University
Marks: 72.38% (First Class)
Organization: Indian Institute of Science Education and Research (IISER) Kolkata
Subjects:
Organization: Idrakpur Primary School, Nadia District Primary School Council, Government of West Bengal
For Communication
For Programming
Research Articles and Proceedings
Conferences and Workshops Attended
Achievements and Awards
Teaching Assistantship
Authors: Yoshita Baruah, Souvik Roy, Suvadip Sinha, Erika Palmerio, Sanchita Pal, Denny M Oliveira, Dibyendu Nandy
Journal: Space Weather, Volume: 22, Issue: 4, Pages: e2023SW003716
DOI: 10.1029/2023SW003716
Abstract: On 3 February 2022, SpaceX launched 49 Starlink satellites, 38 of which unexpectedly de-orbited. Although this event was attributed to space weather, definitive causality remained elusive because space weather conditions were not extreme. In this study, we identify solar sources of the interplanetary coronal mass ejections that were responsible for the geomagnetic storms around the time of launch of the Starlink satellites and for the first time, investigate their impact on Earth's magnetosphere using magnetohydrodynamic modeling. The model results demonstrate that the satellites were launched into an already disturbed space environment that persisted over several days. However, on performing comparative satellite orbital decay analyses, we find that space weather alone was not responsible but conspired together with a low-altitude insertion and low satellite mass-to-area ratio to precipitate this unusual loss. Our work bridges space weather causality across the Sun–Earth system—with relevance for space-based human technologies.
Read more
Authors: Souvik Roy and Dibyendu Nandi
Journal: The Astrophysical Journal Letters, Volume: 950, Issue: 2, Pages: L11
DOI: 10.3847/2041-8213/acd77c
Abstract: To understand the global-scale physical processes behind coronal mass ejection (CME)–driven geomagnetic storms and predict their intensity as a space weather forecasting measure, we develop an interplanetary CME flux rope–magnetosphere interaction module using 3D magnetohydrodynamics. The simulations adequately describe CME-forced dynamics of the magnetosphere including the imposed magnetotail torsion. These interactions also result in induced currents, which are used to calculate the geomagnetic perturbation. Through a suitable calibration, we estimate a proxy of geoeffectiveness—the Storm Intensity index (STORMI)—that compares well with the Dst/SYM-H index. Simulated impacts of two contrasting CMEs quantified by the STORMI index exhibit a high linear correlation with the corresponding Dst and SYM-H indices. Our approach is relatively simple, has fewer parameters to be fine-tuned, and is time efficient compared to complex fluid-kinetic methods. Furthermore, we demonstrate that flux rope erosion does not significantly affect our results. Thus our method has the potential to significantly extend the time window for predictability—an outstanding challenge in geospace environment forecasting—if early predictions of near-Earth CME flux rope structures based on near-Sun observations are available as inputs. This study paves the way for early warnings based on operational predictions of CME-driven geomagnetic storms.
Read more
Authors: Dibyendu Nandy, Yoshita Baruah, Prantika Bhowmik, Soumyaranjan Dash, Sakshi Gupta, Soumitra Hazra, B Lekshmi, Sanchita Pal, Shaonwita Pal, Souvik Roy, Chitradeep Saha, Suvadip Sinha
Journal: Journal of Atmospheric and Solar-Terrestrial Physics, Pages: 106081
DOI: 10.1016/j.jastp.2023.106081
Abstract: Our host star, the Sun, is a middle-aged main sequence G type star whose activity varies. These variations are primarily governed by solar magnetic fields which are produced in the Sun’s interior via a magnetohydrodynamic dynamo mechanism. Solar activity manifests across different timescales, spanning transient phenomena such as flares, energetic particle events and coronal mass ejections to short to long-term modulation of solar irradiance, plasma winds, open flux and cosmic ray flux in the heliosphere. Collectively, these phenomena define space weather and space climate, which impact the state of the near-Earth space environment, the Earth’s magnetosphere, atmosphere and our space-reliant technologies. Understanding physical processes that are at the heart of solar variability and which causally connect the Sun–Earth system is therefore of immense importance to humanity. Such understanding leads to predictions of the impact of solar activity on our planet and provides a window to explore the plasma universe and other star–planet systems, including assessing the habitability of (exo)planets. In this review, based on our research on the solar–terrestrial system and extant scientific literature, we illuminate processes related to the genesis of solar magnetic fields in the Sun’s interior, their emergence and evolution, their manifestation as solar eruptive events, and their eventual impact on the geospace environment mediated via solar winds and storms. We focus on few phenomena that establish causal connections and demonstrate how our current understanding can lead to development of predictive capabilities encompassing the domain of heliophysics.
Read moreNovember 2024
Contributed Poster
November 2023
Contributed Talk
October 2023
Contributed Talk
September 2023
Contributed Talk
July 2023
Invited Talk
April 2023
April 2023
Solicited Talk
March 2023
Contributed Talk
January 2023
Invited Talk
August 2023
Online Attendee
March 2022
Contributed Poster
February 2022
Contributed Talk
January 2022
Contributed Talk