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Using Recurrent Neural Networks to improve initial conditions for a solar wind forecasting model
Filipa S. Barros, Paula A. Graça, J.J.G. Lima, Rui F. Pinto, André Restivo and Murillo Villa Engineering Applications of Artificial Intelligence 133 108266 (2024) https://doi.org/10.1016/j.engappai.2024.108266
The Dynamic Evolution of Solar Wind Streams Following Interchange Reconnection
Coronal Bright Points as Possible Sources of Density Variations in the Solar Corona
Léa Griton, Rui F. Pinto, Nicolas Poirier, Athanasios Kouloumvakos, Michäel Lavarra and Alexis P. Rouillard The Astrophysical Journal 893(1) 64 (2020) https://doi.org/10.3847/1538-4357/ab7b76
Parametric Decay and the Origin of the Low-frequency Alfvénic Spectrum of the Solar Wind
A new model for heating of the Solar North Polar Coronal Hole
E. Devlen, D. Zengin Çamurdan, M. Yardımcı and E. R. Pekünlü Monthly Notices of the Royal Astronomical Society 467(1) 133 (2017) https://doi.org/10.1093/mnras/stx090
The very slow solar wind: Properties, origin and variability
Eduardo Sanchez‐Diaz, Alexis P. Rouillard, Benoit Lavraud, Kevin Segura, Chihiro Tao, Rui Pinto, N. R. Sheeley and Illya Plotnikov Journal of Geophysical Research: Space Physics 121(4) 2830 (2016) https://doi.org/10.1002/2016JA022433
Investigating Alfvénic wave propagation in coronal open-field regions
Takeru K. Suzuki, Shinsuke Imada, Ryuho Kataoka, et al. Publications of the Astronomical Society of Japan 65(5) 98 (2013) https://doi.org/10.1093/pasj/65.5.98
Ion-cyclotron resonance with streaming bi-Maxwellian distribution