Results 101 to 110 of about 1,576,389 (170)

Solar transition region and coronal response to heating rate perturbations [PDF]

open access: yes, 1987
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.
core  

Potential Solar Precursors to Magnetic Switchbacks. [PDF]

open access: yesSpace Sci Rev
Tripathi D   +11 more
europepmc   +1 more source

High-frequency magnetohydrodynamic waves with substantial energy in the solar polar corona. [PDF]

open access: yesNatl Sci Rev
Gao Y   +7 more
europepmc   +1 more source

Electron-Mediated Transport in Space, Astrophysical, and Laboratory Plasmas. [PDF]

open access: yesSpace Sci Rev
Coburn JT   +10 more
europepmc   +1 more source

Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]

open access: yesSol Phys
Woods TN   +9 more
europepmc   +1 more source

The EUV Late-Phase: Statistical Results from 15 Years of Solar Dynamics Observatory Observations. [PDF]

open access: yesSol Phys
Greatorex HJ   +5 more
europepmc   +1 more source

© Author(s) 2008. This work is distributed under the Creative Commons Attribution 3.0 License. Nonlinear Processes in Geophysics

open access: yes, 2014
. 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
core  

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