Selected works from the SWORD Track 1 team

DMSP SSUSI and SSJ Auroral Oval Model Validation

Auroral Oval Model Validation using DMSP-SSUSI

Quantifying and Removing Uncertainties in Ionosphere-Thermosphere Modeling

Propagation of the Solar Wind at Different Scales

Assessing the Uncertainty of Global MHD Simulations

Will Dst Stop Being Useful During Extreme Storms?

Characterizing the Ionospheric Response to Variable Pulsating and Red Diffuse Aurora Precipitation with TREx-ATM

The correlation between off-equator chorus waves and pulsating aurora observed in the same hemisphere

A New Pole-to-Pole Ionospheric Potential Solver

A New Global Potential Solver

Large-Scale Simulated Convection Patterns During 83 Geomagnetic Storms

Statistical Validation of High-Latitude Ion Drifts During 83 Geomagnetic Storms Using DMSP

Modeling the Magnetosphere-Ionosphere-Thermosphere Response to a Hot Flow Anomaly Event on October 30, 2007

Mesoscale Polar Cap Flows and their Impact on Polar Cap Patch Evolution

Multi-Source Data Fusion for Global TEC Map Construction with VISTA Algorithm

Multi-Source Data Fusion for Global TEC Map Construction with VISTA Algorithm

NASA SWORD Center of Excellence: Space weather at LEO

Effects of Different Tidal Forcing on the Thermospheric and Ionospheric State During Different Levels of Geomagnetic Driving Conditions

Modeling the Thermospheric Density During Geomagnetic Storms using the Global Ionosphere Thermosphere Model

Seasonal and Geomagnetic Characterization of F-Region Neutral Winds Over Poker Flat, Alaska

Seasonal and Geomagnetic Characterization of F-Region Neutral Winds Over Poker Flat, Alaska

Artificial mass-loading for protection from major space weather events

Investigating the relative contribution of ion drag to thermospheric wind dynamics in high-latitude regions during a geomagnetic storm: a case study

Studying the onset of reconnection during substorms using an embedded AMR-PIC model

Wave forcing from above and below: detecting traveling atmospheric disturbances and defining gravity waves under differing geomagnetic and terrestrial forcing conditions

Constructing an energy transport map from the solar wind to the inner magnetosphere

Exploring cross polar cap potential in global simulation of the Gannon storm

Revealing magnetosphere feedback on solar wind – magnetosphere coupling via numerical experiment

Geospace energy calculations

Advancements in Modeling the Ionosphere-Thermosphere System's Response to Extreme Geomagnetic Storms

A knowledge-guided deep Gaussian process model for global geomagnetic perturbation forecasting

Numerical tools for investigating foreshock physics and its global impacts

Correcting Empirical Model Densities During Geomagnetic Storms Using Commonly Available Two-Line Element Orbital Data

Effect of SWMF configuration on ground magnetometer power spectra predictions

Results from coupled Geospace-GITM runs

Effects of Improved Auroral Conductance on Magnetotail Dynamics

Impact of collocated auroral precipitation on ionospheric dynamics

The Global Ionosphere Thermosphere Model response to reversed two-cell convection produced during large-scale auroral precipitation in the polar cap

The response of the Global Ionosphere Thermosphere Model to reversed two-cell convection produced during a theta aurora event

Beyond solar storms: theta auroras illuminate the path of solar wind–magnetosphere–ionosphere energy transfer during northward IMF conditions

Assessing Modeled High-Latitude Ionospheric Electrodynamics Using DMSP Observations

DMSP Comparisons with Ionospheric Electrodynamic Patterns

Quantifying Mesoscale Precipitation: Long-term, Large-scale Statistics of Pulsating Aurora Using an ML Identification Algorithm

Meso-scale polar cap flows and their impacts on polar cap patch evolution

Simulating the Impact of Viscosity on Thermospheric Winds and Temperature Structure During Geomagnetic Storms

Assessing High-latitude Electrodynamics: Validation and Characterization of Perturbations in the Coupled Ionosphere-Thermosphere System

Auroral electrojet response to a solar wind density pulse

NASA SWORD Center: from solar wind to surface

Theories and observations of the substorm onset

MHD-AEPIC: Coupled MHD-kinetic simulation of global, meso-, and small-scale magnetospheric phenomena

SWORD Center of Excellence and SWMF: Starlink event 2022 as a case study

Interaction of solar wind transients with the magnetosphere-ionosphere system

Calibrating and fusing ground-based and GOLD-inferred TEC using quantile mapping technique

Next-generation Space Weather Modeling Framework with data assimilation, uncertainty quantification, and machine learning: final year

Exploring the Unusual Day Side Aurora of January 3, 2020

Two-way SWMF-GITM coupling for space weather applications

One Step Closer with GITM: How Lower Atmospheric Tides Control the Ionosphere-Thermosphere

Multi-Scale Density Structures in the Polar Ionosphere: Progress, Challenges, and Outlook

Statistics of Energy Transfer Through the Magnetopause from Spacecraft Observations and Comparison to Global Simulations

The Impact of Solar Wind ULF Fluctuations on Magnetospheric Energetics

The Space Weather Operational Readiness Development (SWORD) Center — an international focal point for orbital space weather forecasting research

The Space Weather Operational Readiness Development (SWORD) Center improving orbital space weather forecasting via model coupling and data assimilation

Improving thermospheric neutral density forecasting with the NOAA/WAM-IPE model

Magnetosphere Energy Transport Analysis for the May 15, 2005 Theta Aurora Event

Numerical modeling of solar wind-magnetosphere interactions: MHD and beyond-MHD models

Exploring solar wind drivers of omega bands

Role of auroral omega bands in storm and substorm processes

Complex polar cap and magnetotail configurations during theta aurora formation

Mesoscale dynamics driven by an external energy pulse during a moderate magnetic storm

Fusing GOLD Satellite-Derived and Ground-Based TEC for Global Ionosphere Analysis

Modeling the Gannon Storm with the SWMF: impacts of input data and model setup