Solar transition region and coronal response to heating rate perturbations [PDF]
The solar transition region is in a dynamic state characterized by impulsively upflowing plasma and continually downflowing plasma. Using numerical simulations, the conjecture that the areas of downflowing plasma are simply the base regions of coronal ...
Mariska, John T.
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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.
europepmc +1 more source
Potential Solar Precursors to Magnetic Switchbacks. [PDF]
Tripathi D +11 more
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High-frequency magnetohydrodynamic waves with substantial energy in the solar polar corona. [PDF]
Gao Y +7 more
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Electron-Mediated Transport in Space, Astrophysical, and Laboratory Plasmas. [PDF]
Coburn JT +10 more
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Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]
Woods TN +9 more
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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 EUV Late-Phase: Statistical Results from 15 Years of Solar Dynamics Observatory Observations. [PDF]
Greatorex HJ +5 more
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Ionospheric Response to the Severe Geomagnetic Storm of 19-21 January 2026 over Almaty (Kazakhstan) According to the Digisonde and GPS Data. [PDF]
Gordiyenko G +6 more
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. We review our recent results of global onedimensional (1-D) MHD simulations for the acceleration of solar and stellar winds. We impose transverse photospheric motions corresponding to the granulations, which generate outgoing Alfvén waves. We treat the
T. K. Suzuki, Coronal Heating
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