Md Nazmus Sakib, Ph.D.
Space Weather Lab, Department of Physics and Astronomy, George Mason University, Fairfax, Virginia, United States of America
Md Nazmus Sakib, Ph.D.
Space Weather Lab, Department of Physics and Astronomy, George Mason University, Fairfax, Virginia, United States of America
Terrestrial Photoelectron Flux Calculation using High-Resolution Photoionization and Photoabsorption Cross Sections and Solar Irradiance
Other Research Topics:
A physics based Ionospheric Model Validation : NEW High Resolution Cross Sections
Atmospheric Ultraviolet Radiation Integrated Code - AURIC - Ionospheric Radiative Calculations at the E-region and above of the Earth (90 km - 150 km and above).
Electron density and Photoelectron fluxes at the upper atmosphere of Earth (data-model validation)
Observations of Ionosphere-Thermosphere electron density composition of Earth by radars (ARECIBO, MILLSTONE HILLS), and satellites (COSMIC-1, 2) using remote sensing technologies.
In-Situ Satellitic Photoelectron flux observations by Atmospheric Explorer - E and Fasr Auroral Snapshot Explorer.
A Novel Technique To detect Non-Radial Rise of Coronal Mass Ejection from the Sun
Observation of Coronal Mass Ejections from the Sun by satellites such as SDO/AIA
Review of Observational Techniques of Atmospheric Gravity Waves in lower atmosphere of Earth by satellites/radars/balloons.
Md Nazmus Sakib (commonly known as "SAKIB") is currently holding PhD in Physics from George Mason University, Fairfax, VA, USA, and working as a reseracher. He began his PhD in 2018 under the supervision of Professors Dr. Bob Meier and Dr. Erdal Yiğit, specializing in terrestrial ionosphere. During his doctoral studies, he contributed to a prestigious NSF-funded science project focusing on long-standing data-model discrepancy in the E-region of the terrestrial ionosphere. His work mainly focused on validation of a physics based ionospheric radiative transfer model to understand the ionospheric structure and variability in terms of electron number density, as well as photoelectron flux energy spectrum variation as a function of altitude. His expertise lies in scientific data analysis using observations by satellites (e.g., Atmospheric Explorer - E, Fast Auroral Snapshot explorer, COSMIC-1-2, TIMED, ICON, GOLD, MAVEN), radars (e.g., Arecibo, Millstone Hills) and empirical models (e.g., IRI). He is also familiar with numerical modeling.
Additionally, he is involved in Solar Physics research with Professor Dr. Jie Zhang(GMU) on a NASA-funded project to study the Coronal Mass Ejection propagation using EUV light by Solar Dynamics Observatory (SDO).
Previously, in Fall 2016, Md Nazmus Sakib moved to the USA to pursue his Master's in Physics and Radio Astronomy at Western Illinois University, Macomb, IL, USA. There, he also worked as a teaching support assistant in the Department of Physics and Astronomy for two years.
He is originally from Bangladesh, and currently resides in Fairfax, Virginia, USA since 2018.
Doctor of Philosophy (May 2025) in Physics, George Mason University, Fairfax, VA, USA, 2025 .
Ph.D. thesis: EXPLORING THE STRUCTURE AND VARIABILITY OF THE TERRESTRIAL IONOSPHERE USING HIGH-RESOLUTION MODEL INPUTS
Master of Science (MS) in Physics and Radio Astronomy, Western Illinois University, Macomb, IL, USA, 2016.
Master of Science in Physics, University of Dhaka, Dhaka, Bangladesh, 2012.
Bachelor of Science in Physics, University of Dhaka, Dhaka, Bangladesh, 2011.
Sponsores of My Research
National Science Foundation
National Aeronautics and Space Administration
George Mason University
Western Illinois University, Physics and Astronomy
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