Results 71 to 80 of about 1,089,572 (146)

Magnetohydrodynamic waves in coronal polar plumes

open access: yes
Polar plumes are cool, dense, linear, magnetically open structures that arise from predominantly unipolar magnetic footpoints in the solar polar coronal holes.

core   +1 more source

Geomagnetic storms driven by ICME- and CIR-dominated solar wind. [PDF]

open access: yes, 2006
The interaction of the solar wind and the Earth's magnetosphere is complex and the phenomenology of the interaction is very different for solar wind dominated by interplanetary coronal mass ejections (ICMEs) compared to solar wind dominated by corotating
Liemohn, M. W.   +8 more
core   +2 more sources

Defining the Middle Corona. [PDF]

open access: yesSol Phys, 2023
West MJ   +41 more
europepmc   +1 more source

Ultra-high-resolution observations of persistent null-point reconnection in the solar corona. [PDF]

open access: yesNat Commun, 2023
Cheng X   +23 more
europepmc   +1 more source

Probing Upflowing Regions in the Quiet Sun and Coronal Holes. [PDF]

open access: yesSol Phys, 2021
Schwanitz C   +7 more
europepmc   +1 more source

Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun. [PDF]

open access: yesLife (Basel), 2023
Kobayashi K   +14 more
europepmc   +1 more source

Dynamics of the Tachocline. [PDF]

open access: yesSpace Sci Rev, 2023
Strugarek A   +4 more
europepmc   +1 more source

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