RF
Rui Ferreira Pinto
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
0000-0001-8247-7168
Employment
Employment history is unavailable.
Education
Education history is unavailable.
Projects & Funding
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SWiFT-FORECAST CNES2018 - 2019
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Solar flare simulations and synthetic X-ray diagnostics CNES2012 - 2014
Publications (194)
- Applying Physics-Informed Neural Networks to Solar Wind Forecasting Save
- FAIR by Design: Advancing the Virtual Space Weather Modelling Center Save
- PARASOL: development of an operational solar storm and high-energy particle forecasting system Save
- From multi-decadal solar wind modelling to real-time forecasting, and on moving away from the ecliptic plane Save
- Testing the flux tube expansion factor - solar wind speed relation with Solar Orbiter data Save
- Calibrating the WSA Model in EUHFORIA Based on Parker Solar Probe Observations Save
- Coronal Models and Detection of the Open Magnetic Field Save
- Advancements in Understanding the Ambient Solar Magnetic Field, Heating, and Spectral Irradiance: A Roadmap Update from COSPAR ISWAT Cluster S2 Save
- Machine Learning and Solar Winds Models, a Story of Surrogation Save
- Solar wind flows across the solar activity cycle, connectivity and plasma signatures on and off the ecliptic plane Save
- Using Recurrent Neural Networks to improve initial conditions for a solar wind forecasting model Save
- Calibrating the WSA model in EUHFORIA based on PSP observations Save
- On the Origin of the Sudden Heliospheric Open Magnetic Flux Enhancement During the 2014 Pole Reversal Save
- Solar wind flows across the solar activity cycle, connectivity and plasma signatures on and off the ecliptic plane Save
- Neural Networks for Surrogate Models of the Corona and Solar Wind Save
- Enhancing Triangulation of Interplanetary Type III Bursts through Wavevector Correction Save
- Helio1D modeling of temporal variation of solar wind: Interfacing between MULTI-VP and 1D MHD for future operational forecasting at L1 Save
- Revealing the origin of the December 2022 disappearing solar wind event Save
- Coronal Models and Detection of Open Magnetic Field Save
- Linking the measured solar wind speed to the modelled coronal magnetic field Save