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Found 4 papers, 2 papers with code
Automatic Detection of Interplanetary Coronal Mass Ejections in Solar Wind In Situ Data
Additionally, it produced reasonable results on datasets with fewer features and smaller training sets from Wind, STEREO-A and STEREO-B with True Skill Statistics of 0. 56, 0. 57 and 0. 53, respectively.
Radial Evolution of the April 2020 Stealth Coronal Mass Ejection between 0.8 and 1 AU -- A Comparison of Forbush Decreases at Solar Orbiter and Earth
The very slow (~350 km/s) stealth CME caused a FD with an amplitude of 3 % in the low-energy cosmic ray measurements at HET and 2 % in a comparable channel of the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) on the Lunar Reconnaissance Orbiter, as well as a 1 % decrease in neutron monitor measurements.
Solar and Stellar Astrophysics Earth and Planetary Astrophysics Space Physics
Prediction of the in situ coronal mass ejection rate for solar cycle 25: Implications for Parker Solar Probe in situ observations
The Parker Solar Probe (PSP) and Solar Orbiter missions are designed to make groundbreaking observations of the Sun and interplanetary space within this decade.
Solar and Stellar Astrophysics Earth and Planetary Astrophysics Space Physics
Forward modeling of coronal mass ejection flux ropes in the inner heliosphere with 3DCORE
It combines a novel semi-empirical model of CME flux rope magnetic fields (3-Dimensional Coronal ROpe Ejection or 3DCORE) with solar observations and in situ magnetic field data from along the Sun-Earth line.
Solar and Stellar Astrophysics Earth and Planetary Astrophysics
