Turn on the super-elastic collision nature of coronal mass ejections through low approaching speed. [PDF]
Sci Rep, 2016 Shen F, Wang Y, Shen C, Feng X.
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The Sun’s magnetized plasma atmosphere is the source of various forms of activity, the most dramatic of which are coronal mass ejections (CMEs). These ejections are a bulk expulsion of plasma and magnetic field that travel out into the heliosphere ...
Green, Lucie M
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Space-Weather Utilities for Research and Forecasting (SURF): A Tool for Investigating Hydrodynamic Aspects of Solar Wind and Coronal Mass Ejection Expansion and Evolution. [PDF]
Sol PhysOwens MJ, Barnard LA.
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Back reaction of the untwisting solar corona scars sunspots. [PDF]
Sci AdvXing C, Cheng X, Aulanier G, Ding M.
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The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]
Nat CommunErvin T, Nakhleh AJ, Bharati Das S.
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Ubiquitous Kelvin-Helmholtz instabilities driving plasma mixing on the Sun. [PDF]
NatureKuridze D +11 more
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SSTrack: An Automatic Sunspot Identification and Tracking Algorithm to Support the Measurement of Sunspot Rotation. [PDF]
Sol PhysProverbs C, Brown D.
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Self-consistent numerical simulations for the formation and dynamics of solar prominences. [PDF]
Nat AstronZessner LM +3 more
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Observations of successive CMEs and their successive Type II solar radio bursts in the corona. [PDF]
Sci RepVasanth V.
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Coronal bright points: magnetic topology and mini coronal mass ejections
Coronal bright points (small-scale loop systems) in the solar atmosphere were studied for more than 4 decades but the physical mechanism responsible for their formation and evolution is still unknown. I will present two recent studies.
Madjarska, M.
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