CA
Charles Arge
NASA/Goddard Space Flight Center, University of Delaware
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
0000-0001-9326-3448
Employment
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NASA/Goddard Space Flight Center Supervisory Research Astrophysicist2016 - Present
Education
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University of Delaware Ph.D.1997 - Present
Projects & Funding
Projects & funding information is unavailable.
Publications (42)
- Solar Orbiter’s Far-side Magnetogram Impacts on Coronal Holes and Solar Wind Predictions Save
- Advancing Heliophysics and Space Weather Modeling through Open Science Save
- Synoptic Maps of Solar Magnetic Field and Open Magnetic Flux Save
- The Effect of Spatial Resolution on the Wang–Sheeley–Arge Model Unsigned Open Flux Prediction Save
- Quantitative Image-based Validation Framework for Assessing Global Coronal Magnetic Field Models Save
- Advancing Heliophysics and Space Weather Modeling through Open Science Save
- Improving the Arrival Time Estimates of Coronal Mass Ejections by Using Magnetohydrodynamic Ensemble Modeling, Heliospheric Imager Data, and Machine Learning Save
- The Quasi-radial Field-line Tracing (QRaFT): An Adaptive Segmentation of the Open-flux Solar Corona Save
- Why Do Solar Wind Models Get It Wrong? Understanding the Capabilities of Time-dependent Solar Wind Simulations Save
- Neural Enhancement of the Traditional Wang–Sheeley–Arge Solar Wind Relation Save
- Incorporating Magnetic-Field Characteristics into EUV-Based Automated Segmentation of Coronal Holes Save
- Ensemble Modeling of the Solar Wind Flow with Boundary Conditions Governed by Synchronic Photospheric Magnetograms. I. Multipoint Validation in the Inner Heliosphere Save
- What Causes Errors in Wang–Sheeley–Arge Solar Wind Modeling at L1? Save
- Deriving the Coronal Separatrix‐Web With the WSA Model Save
- Quantifying Uncertainties in Solar Wind Forecasting due to Incomplete Solar Magnetic Field Information Save
- Using solar wind data assimilation results to drive dynamic solar wind models. Save
- Open-source Flux Transport (OFT). I. HipFT–High-performance Flux Transport Save
- Improved Tomographic Reconstruction of 3D Global Coronal Density from STEREO/COR1 Observations Save
- Deriving the Coronal Separatrix-web with the WSA Model Save
- Magnetic Field-Constrained Ensemble Image Segmentation of Coronal Holes in Chromospheric Observations Save