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Eruptions from coronal hole bright points: Observations and non-potential modelling
Maria S. Madjarska, Klaus Galsgaard, Duncan H. Mackay, Kostadinka Koleva and Momchil Dechev Astronomy & Astrophysics 643 A19 (2020) https://doi.org/10.1051/0004-6361/202038287
Stellar coronal mass ejections – II. Constraints from spectroscopic observations
P Heinzel, E W Guenther, M Leitzinger and P Odert Monthly Notices of the Royal Astronomical Society 494(3) 3766 (2020) https://doi.org/10.1093/mnras/staa1021
Models and data analysis tools for the Solar Orbiter mission
First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-correlation Analysis
Beili Ying, Alessandro Bemporad, Silvio Giordano, Paolo Pagano, Li Feng, Lei Lu, Hui Li and Weiqun Gan The Astrophysical Journal 880(1) 41 (2019) https://doi.org/10.3847/1538-4357/ab2713
Formation of Coronal Mass Ejections in the Solar Corona and Propagation of the Resulting Plasma Streams in the Heliosphere
Forward Modeling of SDO/AIA and X-Ray Emission from a Simulated Flux Rope Ejection
Xiaozhou 小舟 Zhao 赵, Chun Xia, Tom Van Doorsselaere, Rony Keppens and Weiqun Gan The Astrophysical Journal 872(2) 190 (2019) https://doi.org/10.3847/1538-4357/ab0284
Diagnostics of the Prominence Plasma from Hα and Mg ii Spectral Observations
Guiping Ruan, Sonja Jejčič, Brigitte Schmieder, Pierre Mein, Nicole Mein, Petr Heinzel, Stanislav Gunár and Yao Chen The Astrophysical Journal 886(2) 134 (2019) https://doi.org/10.3847/1538-4357/ab4b50
Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test
A new technique for observationally derived boundary conditions for space weather
Paolo Pagano, Duncan Hendry Mackay and Anthony Robinson Yeates Journal of Space Weather and Space Climate 8 A26 (2018) https://doi.org/10.1051/swsc/2018012
Origin and Ion Charge State Evolution of Solar Wind Transients during 4 – 7 August 2011
ERUPTING FILAMENTS WITH LARGE ENCLOSING FLUX TUBES AS SOURCES OF HIGH-MASS THREE-PART CMEs, AND ERUPTING FILAMENTS IN THE ABSENCE OF ENCLOSING FLUX TUBES AS SOURCES OF LOW-MASS UNSTRUCTURED CMEs