8 citations · 10 across the 3 of their papers we have counts for
3 papers
astro-ph.SR2025
Understanding the complex morphology of a CME: multi-view analysis and numerical modeling
Cecilia Mac Cormack, Abril Sahade, Angelos Vourlidas +3
Although all coronal mass ejections (CMEs) that propagate into the heliosphere should contain a magnetic flux rope (MFR) component, the majority do not exhibit the expected white-l…
astro-ph.SR2025★ 2 cited
Helmet streamer influence on the evolution of magnetic flux ropes
M. Cécere, P. F. Wyper, G. Krause +2
Context: Solar eruptions are crucial for space weather studies. Understanding the mechanisms influencing their evolution is key to improving predictions of their geoeffectiveness.…
astro-ph.SR2024★ 8 cited
Analysis of solar eruptions deflecting in the low corona: influence of the magnetic environment
A. Sahade, A. Vourlidas, C. Mac Cormack
Coronal mass ejections (CMEs) can exhibit non-radial evolution. The background magnetic field is considered the main driver for the trajectory deviation relative to the source regi…