On the Acceleration of the Young Solar Wind from Different Source Regions
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
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]
Nitta NV +16 more
europepmc +1 more source
Quantitative Image-based Validation Framework for Assessing Global Coronal Magnetic Field Models
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]
Zhang J +18 more
europepmc +1 more source
Cross Helicity and the Helium Abundance as an In Situ Metric of Solar Wind Acceleration
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]
Vidotto AA.
europepmc +1 more source
A Model for Flux Rope Formation and Disconnection in Pseudostreamer Coronal Mass Ejections
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]
Davoudifar P +6 more
europepmc +1 more source
Nine Outstanding Questions of Solar Wind Physics. [PDF]
Viall NM, Borovsky JE.
europepmc +1 more source

