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A global 2.5-dimensional three fluid solar wind model with alpha particles
Bo Li
*
,
Xing Li
, Nicolas Labrosse
*
Corresponding author for this work
Department of Physics
Research output
:
Contribution to journal
›
Article
›
peer-review
18
Citations (Scopus)
Overview
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Dive into the research topics of 'A global 2.5-dimensional three fluid solar wind model with alpha particles'. Together they form a unique fingerprint.
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Earth and Planetary Sciences
Abundance
50%
Agreement
16%
Alpha Radiation
100%
Boundary
16%
Core
33%
Corona
16%
Coulomb Collision
33%
Coupling
33%
Drag
16%
Drain
16%
Electron
33%
Energy Flux
16%
Friction
16%
Heat Flux
33%
Heating
33%
Impact
16%
In Situ Measurement
16%
Ion
33%
Magnetic Field
50%
Model
33%
Need
16%
Observation
16%
Particle
16%
Plasma
16%
Play
16%
Proton
66%
Region
33%
Settling
33%
Solar Wind
83%
Species
33%
Speed
33%
Sun
16%
Timescale
16%
Wind
33%
Physics
Alpha Radiation
100%
Cores
33%
Coronas
16%
Drag
16%
Friction
16%
Heating
33%
Impact
16%
in Situ Measurement
16%
Independent Variables
16%
Ion
33%
Magnetic Fields
50%
Model
33%
Particle
16%
Protons
66%
Region
33%
Sensory Perception
16%
Settling
33%
Solar Wind
83%
Speed
33%