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Viacheslav Sadykov
Georgia State UniversityMeeting roles in:
Modeling-Based Diagnostics of Propagating High-Frequency Acoustic Waves in the Lower Solar Atmosphere
Velocity Distributions and Kinetic Wave Activity in Space Plasma: Theory, Simulation, and Machine Learning Poster
Identification of Ion-Kinetic Instabilities in Solar Wind Plasma with Machine Learning: from Hybrid-PIC Simulations to Observational Data
Importance of Alpha Particle Beams in Driving Ion Scale Waves in Solar Wind Close to the Sun
Modeling Ion-Scale Waves and Kinetic Instabilities in Proton-Alpha Solar Wind Plasma Observed by Parker Solar Probe
Monitoring and Forecasting Space and Terrestrial Weather with Ground-Based Measurements of Cosmic Rays Poster
East–West Asymmetry in Muon Flux as a Probe of Geomagnetic Field Changes
Development of a Low-Cost, Temperature-compensated Readout System for Global Muon Detector Network
Enhancing Radiation Exposure Prediction at Aviation Altitudes Using Machine Learning and Cosmic Ray Muon Measurements
Preliminary Analysis of Large Forbush Decreases in June 2025 Using Observations from the gLOWCOST Detector Network
Prediction of Solar Transient Events: Data-Driven, Physics-Based, and Hybrid Approaches I Poster
Evaluating the Effectiveness of Active Region/Polarity Inversion Line Segmentation with Heliophysics Foundation Models
The Role of Flare Ribbon and 3D Magnetic Field Topology in Flare Eruptivity
Comparative Analysis of 10 - 50 MeV Solar Proton Events at Lagrange Point 1 and the Geostationary Orbit
May 2024 Solar Energetic Particle Storms: Peculiarities and Predictability
Intertwining Physics-Based CME Modeling and Machine Learning for L1 Prediction of Interplanetary Magnetic Field
Prediction of Solar Transient Events: Data-Driven, Physics-Based, and Hybrid Approaches II Oral
Utilizing Large-Scale Heliophysics Foundation Models for Solar Flare Forecasting
Enhancing the SWAN-SF Flare Forecasting Dataset’s Usefulness
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