Space Research Laboratory
- COMPARATIVE MORPHOLOGY OF SOLAR RELATIVISTIC PARTICLE EVENTS (2015)
- Comprehensive Characterization of Solar Eruptions with Remote and In-Situ Observations, and Modeling: The Major Solar Events on 4 November 2015 (2020)
- Connecting remote and in situ observations of shock-accelerated electrons associated with a coronal mass ejection (2024)
- Connecting solar flare hard X-ray spectra to in situ electron spectra A comparison of RHESSI and STEREO/SEPT observations (2021)
- Connecting the Properties of Coronal Shock Waves with Those of Solar Energetic Particles (2019)
- Consistency of the average flux of solar energetic particles over different timescales up to mega-years (2024)
- Consistency of the average flux of solar energetic particles over timescales of years to megayears (2023)
- CORBES: radiation belt survey with international small satellite constellation (2025)
- Coronal Conditions for the Occurrence of Type II Radio Bursts (2021)
- Correcting for interplanetary scattering in velocity dispersion analysis of solar energetic particles (2015)