Results 71 to 80 of about 5,952,631 (141)
Modeling the Transport of Solar Energetic Particles in a Corotating Interaction Region
We present a new three-dimensional (3D) magnetohydrodynamic (MHD) model and a new 3D energetic particle transport (EPT) model. The 3D MHD model numerically solves the ideal MHD equations using the relaxing total variation diminishing scheme.
Y.-S. Zhong, G. Qin, S.-S. Wu
doaj +1 more source
The paper presents the results of MHD modeling of corotating interaction regions (CIRs) at distances of 0.1 AU from the Sun (inner boundary) to much larger distances (20–30 AU) in two variants in which the magnetic field on the photosphere (1) is ...
Pavlov Dmitry +6 more
doaj +1 more source
We use a 3D Monte Carlo radiative transfer code to study the polarimetric and photometric variability from stationary corotating interaction regions (CIR) in the wind of massive stars. Our CIRs are approximated by Archimedean spirals of higher (or lower)
Carlos-Leblanc, Danny +3 more
core +1 more source
Recent multiwavelength observations of young solar analogs suggest that the young Sun in the first 600 Myr was a magnetically active star that produced an X-ray and extreme-UV bright corona, fast, massive stellar wind, and energetic eruptive events ...
Dibyendu Sur, Vladimir S. Airapetian
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Fractal Dimension Analysis of Earth Magnetic Field during 26 August 2018 Geomagnetic Storm. [PDF]
Wawrzaszek A +4 more
europepmc +1 more source
Context. Energetic particle enhancements that are associated with corotating interaction regions (CIRs) are typically believed to arise from the sunward propagation of particles that are accelerated by CIR-driven shocks beyond 1 AU.
P. Bochsler +13 more
core +1 more source
Energetic particle acceleration and transport with the novel Icarus + PARADISE model
With the rise of satellites and mankind’s growing dependence on technology, there is an increasing awareness of space weather phenomena related to high-energy particles.
Husidic Edin +4 more
doaj +1 more source
Comparing and Contrasting the Properties of the Inner Heliosphere for the Three Most Recent Solar Minima. [PDF]
Riley P +4 more
europepmc +1 more source
Solar Orbiter survey of inner heliosphere low energy ions (greater than ∼100 keV/nucleon), 2020–2025
Context. The Solar Orbiter spacecraft cruised in the inner heliosphere from April 2020 to December 2025, moving between ∼0.3–1.0 au radial distance. The Energetic Particle Detector (EPD) suite operated continuously during this period. Aims.
Mason G. M. +6 more
doaj +1 more source
The Plasma Environment of Comet 67P/Churyumov-Gerasimenko. [PDF]
Goetz C +26 more
europepmc +1 more source

