Results 91 to 100 of about 205 (182)

On the Acceleration of the Young Solar Wind from Different Source Regions

open access: yesThe Astrophysical Journal Letters
The acceleration of the young solar wind is studied using the first 17 encounters of the Parker Solar Probe. We identify wind intervals from different source regions: coronal hole (CH) interiors, streamers, and low-Mach-number boundary layers (LMBLs), i ...
Yiming Jiao   +4 more
doaj   +1 more source

Radial Evolution of a Density Structure within a Solar Wind Magnetic Sector Boundary

open access: yesThe Astrophysical Journal
This study focuses on a radial alignment between Parker Solar Probe (PSP) and Solar Orbiter (SolO) on 2021 April 29 (during a solar minimum), when the two spacecraft were, respectively, located at ∼0.075 and ∼0.9 au from the Sun. A previous study of this
Etienne Berriot   +5 more
doaj   +1 more source

Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections. [PDF]

open access: yesSpace Sci Rev, 2021
Nitta NV   +16 more
europepmc   +1 more source

Quantitative Image-based Validation Framework for Assessing Global Coronal Magnetic Field Models

open access: yesThe Astrophysical Journal
Coronagraph observations provide key information about the orientation of the Sun’s magnetic field. Previous studies used various algorithms to segment quasi-radial features in coronagraph images and approximate their local plane-of-sky (POS) geometry ...
Christopher E. Rura   +5 more
doaj   +1 more source

Earth-affecting solar transients: a review of progresses in solar cycle 24. [PDF]

open access: yesProg Earth Planet Sci, 2021
Zhang J   +18 more
europepmc   +1 more source

Cross Helicity and the Helium Abundance as an In Situ Metric of Solar Wind Acceleration

open access: yesThe Astrophysical Journal Letters
The two-state solar wind paradigm is based on observations showing that slow and fast solar wind have distinct properties like helium abundances, kinetic signatures, elemental composition, and charge-state ratios. Nominally, the fast wind originates from
B. L. Alterman, Raffaella D’Amicis
doaj   +1 more source

The evolution of the solar wind. [PDF]

open access: yesLiving Rev Sol Phys, 2021
Vidotto AA.
europepmc   +1 more source

A Model for Flux Rope Formation and Disconnection in Pseudostreamer Coronal Mass Ejections

open access: yesThe Astrophysical Journal
Coronal mass ejections (CMEs) from pseudostreamers represent a significant fraction of large-scale eruptions from the Sun. In some cases, these CMEs take a narrow jet-like form reminiscent of coronal jets; in others, they have a much broader fan-shaped ...
P. F. Wyper   +5 more
doaj   +1 more source

Development of a local empirical model of ionospheric total electron content (TEC) and its application for studying solar-ionospheric effects. [PDF]

open access: yesSci Rep, 2021
Davoudifar P   +6 more
europepmc   +1 more source

Nine Outstanding Questions of Solar Wind Physics. [PDF]

open access: yesJ Geophys Res Space Phys, 2020
Viall NM, Borovsky JE.
europepmc   +1 more source

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