Results 121 to 130 of about 205 (182)

The Physical Origin of Periodic Density Structures in the Solar Wind: Coronal Streamers as Magnetohydrodynamic Resonators

open access: yes
We present a comprehensive physical model explaining the origin of Periodic Density Structures (PDS) observed in white-light coronagraphs with characteristic periods of approximately 45, 80, and 120 minutes. Through systematic investigation of potential resonant cavities in the solar atmosphere, we demonstrate that traditional large-scale cavities ...
openaire   +2 more sources

Mapping the Sun's coronal magnetic field using the Zeeman effect. [PDF]

open access: yesSci Adv
Schad TA   +11 more
europepmc   +1 more source

Exceptionally gigantic aurora in the polar cap on a day when the solar wind almost disappeared. [PDF]

open access: yesSci Adv
Hosokawa K   +6 more
europepmc   +1 more source

Assessing the Quality of Models of the Ambient Solar Wind. [PDF]

open access: yesSpace Weather, 2018
MacNeice P   +13 more
europepmc   +1 more source

Helios Observations of Quasiperiodic Density Structures in the Slow Solar Wind at 0.3, 0.4, and 0.6 AU. [PDF]

open access: yesJ Geophys Res Space Phys, 2019
Di Matteo S   +5 more
europepmc   +1 more source

Explosive Magnetotail Activity. [PDF]

open access: yesSpace Sci Rev, 2019
Sitnov M   +15 more
europepmc   +1 more source

Magnetic Nulls and Super-radial Expansion in the Solar Corona. [PDF]

open access: yesAstrophys J Lett, 2017
Gibson SE   +7 more
europepmc   +1 more source

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