Institute for Space Weather Sciences

Chromospheric Magnetic Field: A Comparison of He I 10830 Å Observations with Nonlinear Force-free Field Extrapolation

Eruptions Observed by the Full Sun Imager (FSI) - a Telescope of the Extreme Ultraviolet Imager (EUI) Instrument Onboard Solar Orbiter

SPI3S: SPectral Irradiance of a 3d Sun

ML-Eco Fi: A Machine Learning Ecosystem for Automatic Analysis of Solar Filaments

The Magnetic Corona and the Promise of Coronagraphic Magnetometry 

On Inverting Solar Coronal Vector Magnetic Fields from Infrared Observations

Aditya L1: India’s Space Observatory to Study the Sun

What Does a Magnetic Flux Rope Look Like?

Erupting Solar Magnetic Flux Ropes and the Bz Challenge: Understanding Details of CME Propagation in the Interplanetary Media

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Emission Characteristics and Evolution of Solar Filaments

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Implications of Electron Beam Propagation on Flare Energetics

Solar and Heliospheric Modeling and Forecasting Using WSA

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A review of the M6.5 Flare on June 22, 2015

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Numerical Modeling of Flare Loop-top Regions

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Modeling the Solar Dynamo: Past, Present and Future

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Simulations and Observations of Active Region Magnetic Flux Emergence

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On the Ribbon Front:  Chromospheric Response to the Initial Beam of Electrons

The latest low energy results from the Alpha Magnetic Spectrometer (AMS) on the International Space Station 

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The Making of the Space Weather Modeling Framework

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Citizen Science Contributions to Solar-Terrestrial Physics

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Machine Learning for Space Weather Analytics

Solar Energetic Particles Associated with Fast Coronal Mass Ejections

Machine Learning-Enabled Orbit Prediction and Earth Observation

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Turbulence and the Heating of the Solar Corona

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Observational Signatures of Small-Scale Magnetic Flux Ropes at 1 AU and Their Magnetic Connectivity to the Sun

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Past and Future of Data-Constrained/Driven MHD simulations of Solar Eruptions

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Self-Consistent Modeling of Cross-Energy Coupling in the Inner Magnetosphere

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The Early Stages of CME-Driven Shocks: from Remote Observations to SEPs

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Type III Radio Burst Fine Structure: Electrons, Turbulence and Waves

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Electron Acceleration and the Development of Power-law Energy Spectra in Magnetic Reconnection in a Force-free Current Sheet

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Data-Constrained Modeling of Eruptions in the Solar Corona: Incorporating state-of-the-art science into the next generation of space weather modeling tools

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Models of the Energy Buildup and Explosive Release in Flares/CMEs

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Radio-based Studies of Solar Flares: Looking Ahead to the Next Solar Maximum in 2025

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Eruptive Solar Flares with Parallel and Circular Ribbons

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ML Efforts on Understanding and Predicting Solar Flares

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Advancing the Coronal Heating Problem with Microwave Gyro Emission

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Hardware-software Codesign for Accelerating Data Science at the Edge

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Coronal Jets – the Key to Understanding Solar Eruptions and Plumes

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The Interplanetary Propagation of Coronal Mass Ejections: Recent Development and Path Forward

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Diagnostics New and Old for a Dynamic Chromosphere

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Measurement of Magnetic Field and Relativistic Electrons along a Solar Flare Current Sheet

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Magnetic Reconnection Rate & X-line Spread in Collisionless Plasmas  

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The Solar Corona from Within: Overview of WISPR Science Results & Future Outlook

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Magnetic Connectivity During the Early PSP Encounters

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High Resolution Observations of Solar Flares   

(Link to talk)