Analysis of the September 6, 2011 coronal wave with the SOLERwave multi-sector method reveals over 40% speed variation (750-1500 km/s) between northward and northwestward segments, attributed to differences in magnetosonic speed from an MHD solution.
2017 Acceleration and Propagation of Solar Energetic Particles.Space Sci
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First estimates of radiation doses during extreme SEP events, derived from radionuclide data under the assumption of single-event causes with modern-like spectra and geomagnetic conditions.
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Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool
Analysis of the September 6, 2011 coronal wave with the SOLERwave multi-sector method reveals over 40% speed variation (750-1500 km/s) between northward and northwestward segments, attributed to differences in magnetosonic speed from an MHD solution.
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Radiation doses during extreme solar energetic particle events
First estimates of radiation doses during extreme SEP events, derived from radionuclide data under the assumption of single-event causes with modern-like spectra and geomagnetic conditions.