Hello, I am

Dr. Souvik Roy

Who am I ?

A Student, Science Enthusiast and Postdoctoral Scholar Located In Our Lovely Earth



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.

Professional Information

Areas of Interest

Solar-Terrestrial Physics

Heliophysics and the coupled Sun-Earth system.


Multi-fluid Magnetohydrodynamics

Global plasma simulations and high-performance computing.


Space Weather

Physics-based forecasting of geomagnetic disturbances.


Magnetosphere-Ionosphere Coupling

Ionospheric outflow, plasma transport, and magnetospheric dynamics.


Plasma Sheet Dynamics

Heavy-ion transport, composition, and energy evolution.


Coronal Mass Ejections and Geomagnetic Storms

Solar eruptions, their impact on planetary magnetospheres, Storm-time dynamics, ring current evolution, and geomagnetic activity.


Computational Space Physics

Scientific computing, numerical modeling, and data-driven analysis.


Satellite Data Analysis

Multi-mission observations and validation of numerical simulations.


Lunar Space Environment

Solar wind interaction with the Moon and planetary plasma environments.


Scientific Visualization

Visualization, analysis, and interpretation of large-scale simulation data.


My Resume

Education

PhD in Astrophysics and Space Science

2018 - 2024

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.


Masters in Physics

2015 - 2017

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


Bachelors in Physics (Honours)

2012 - 2015

Affiliation: Rishi Bankim Chandra College, Naihati, India
University: West Bengal State University

Marks: 72.38% (First Class)

Teaching Experience

Teaching Assistant

2020 - 2022

Organization: Indian Institute of Science Education and Research (IISER) Kolkata

Subjects:

  • Intermediate Electricity Magnetism (PH3202)
    • Instructor: Prof. Rajesh Kumble Nayak
      • Spring 2020

  • Introductory Astrophysics (PH4102)
    • Instructor: Prof. Dibyendu Nandi
      • Autumn 2020
      • Autumn 2021
      • Autumn 2022

  • Fluid and Magnetohydrodynamics (SS4201)
    • Instructor: Prof. Dibyendu Nandi
      • Spring 2021
      • Spring 2022


Assistant Teacher

2017 - 2018

Organization: Idrakpur Primary School, Nadia District Primary School Council, Government of West Bengal

Skills & Languages

For Communication

English
Bangla (Bengali) - বাংলা
Hindi - हिन्दी
Spanish - español

Expertise

Astrophysics and Fluid Dynamics
Computational Magnetohydrodynamics
High Performance Computing
Sattelite Data Analysis
Image Analysis
Data Visualisation
Coordinate Geometry

Skills & Languages

For Programming

Python
Matlab
C
Fortran
MAGE (Software)
PLUTO (Software)
Linux/Bash
Latex and basic Office tools
VisIt (Software)
Paraview (Software)
Kdenlive (Software)

10+

Research Articles and Proceedings

20+

Conferences and Workshops Attended

12+

Achievements and Awards

6+

Teaching Assistantship

Notable Works

The loss of Starlink satellites in February 2022: How moderate geomagnetic storms can adversely affect assets in low‐earth orbit
The loss of Starlink satellites in February 2022: How moderate geomagnetic storms can adversely affect assets in low‐earth orbit

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
A Time-efficient, Data-driven Modeling Approach for Predicting the Geomagnetic Impact of Coronal Mass Ejections
A Time-efficient, Data-driven Modeling Approach for Predicting the Geomagnetic Impact of Coronal Mass Ejections

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
Causality in heliophysics: Magnetic fields as a bridge between the Sun’s interior and the Earth’s space environment
Causality in heliophysics: Magnetic fields as a bridge between the Sun’s interior and the Earth’s space environment

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 more

সহজ কথা, সহজ করে, বলি না তো সহজে!
বলি তারে কঠিন করে, যাতে ঢোকে মগজে..

Recent Conferences and Workshops

20th European Space Weather Week

November 2024

Contributed Poster

American Geophysical Union Fall Meeting 2022

December 2023

NASA ADS: FMSH11G FMSH21D

19th European Space Weather Week

November 2023

Contributed Talk

4th Eddy Cross-Disciplinary Symposium

October 2023

Contributed Talk

UK Space Weather and Space Environment Meeting

September 2023

Contributed Talk

Fourth Aditya L1 Support Cell Workshop 2023

July 2023

Invited Talk

European Geosciences Union (EGU) General Assembly 2023

April 2023

DOI: 10.5194/egusphere-egu23-16801

USO-PRL Solar Physics Workshop (USPW-2023)

April 2023

Solicited Talk

41th Annual Meeting of the Astronomical Society of India

March 2023

Contributed Talk

NASA Heliophysics Science Division (HSD) Seminar

January 2023

Invited Talk

American Geophysical Union Fall Meeting 2022

December 2022

NASA ADS: 2022AGUFMSM32D1746R

NASA Heliophysics Summer School 2022

August 2023

Online Attendee

44th COSPAR Scientific Assembly

July 2022

NASA ADS: 2022cosp...44.1392R

40th Annual Meeting of the Astronomical Society of India

March 2022

Contributed Poster

15th Quadrennial Solar-Terrestrial Physics symposium

February 2022

Contributed Talk

21st National Space Science Symposium (NSSS - 2022)

January 2022

Contributed Talk

American Geophysical Union Fall Meeting 2021

December 2021

DOI: 10.1002/essoar.10511097.1

European Geosciences Union (EGU) General Assembly 2021

April 2021

DOI: 10.5194/egusphere-egu21-8863

মুখ ঢেকেছি বিজ্ঞাপনে, রেখেছি তবু খুব যতনে
মনের নরমখানি।
সহজ, কিন্তু জটিল ভারী! এড়িয়ে বাঁচা ঝকমারী —
হাসির হাতছানি।

Awards and Achivements

Senior Research Fellowship from Council of Scientific & Industrial Research (CSIR)
2020
Junior Research Fellowship from Council of Scientific & Industrial Research (CSIR), June 2017
2018
West Bengal Government Swami Vivekananda Merit cum Means (SVMCM) Scholarship
2015 - 2017
2nd Rank Holder in M.Sc in Physics in West Bengal State University
2017
Avik Mukherjee Memorial Award, Rishi Bankim Chandra College, (College Topper in Honours)
2015
10th Rank Holder in B.Sc in Physics in West Bengal State University
2015
Rishi Bankim Medha Puroshkar (Topper in B.Sc Honours)
2015
Rishi Bankim Chandra College Award (Topper Physics Honours)
2015
Nagendra Nath Pal Memorial Award (Topper Physics Honours)
2015
Indian Oil (IOCL) Scholarship For Higher Secondary Studies
2010 - 2012
West Bengal Government Merit Cum Means Scholarship
2010 - 2012
West Bengal Government Merit Cum Means Scholarship
2008 - 2010

ফেরার তাড়া ছিল, তারা দেখা হয়নি তার
কি জানি, কোনদিনও, সুযোগ হবে কি আর!
আড়িতেই ছুঁয়ে ছিল, সেটুকুই থাক তবে।
স্মৃতির পাতাই সই, মোলাকাৎ ধবধবে!

Get in touch

Telehone :
+1 (310) ZLI-OG-16; +91 (WRE) DL-130-RL
Address :
520 Portola Plaza,
Los Angeles, CA 90095, USA
Email :
souvik[at]atmos[dot]ucla[dot]edu
mail2me[dot]souvik[at]gmail[dot]com