Diagnosis of Coronal Mass Ejections through Local and Global Dimmings
Coronal dimmings are localized sharp reductions in soft X-ray and extreme ultraviolet (EUV) emission at the early expansion phase of coronal mass ejections (CMEs). Such local dimmings have global responses, known as Sun-as-a-star or global dimmings. Here,
Tao Ding, Jun Zhang, Ting Li
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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]
Owens MJ, Barnard LA.
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Back reaction of the untwisting solar corona scars sunspots. [PDF]
Xing 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]
Ervin T, Nakhleh AJ, Bharati Das S.
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Ubiquitous Kelvin-Helmholtz instabilities driving plasma mixing on the Sun. [PDF]
Kuridze D +11 more
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SSTrack: An Automatic Sunspot Identification and Tracking Algorithm to Support the Measurement of Sunspot Rotation. [PDF]
Proverbs C, Brown D.
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The structure of a complex, asymmetric coronal mass ejection revealed by 17 spacecraft across the inner heliosphere. [PDF]
Luspay-Kuti A +30 more
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Self-consistent numerical simulations for the formation and dynamics of solar prominences. [PDF]
Zessner LM +3 more
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Potential Solar Precursors to Magnetic Switchbacks. [PDF]
Tripathi D +11 more
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Observations of successive CMEs and their successive Type II solar radio bursts in the corona. [PDF]
Vasanth V.
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