Browsing by Subject "Methods: numerical"
Now showing items 1-5 of 5
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Cosmic-ray transport in heliospheric magnetic structures. II. Modeling particle transport through corotating interaction regions
(IOP, 2017)The transport of cosmic rays (CRs) in the heliosphere is determined by the properties of the solar wind plasma. The heliospheric plasma environment has been probed by spacecraft for decades and provides a unique opportunity ... -
Determining pitch-angle diffusion coefficients from test particle simulations
(IOP Publishing, 2016)The transport and acceleration of charged particles in turbulent media are topics of great interest in space physics and interstellar astrophysics. These processes are dominated by the scattering of particles off magnetic ... -
Exploiting morphological data from Pulsar Wind Nebulae via a spatiotemporal leptonic transport code
(Oxford Univ Press, 2020)The next era of ground-based Cherenkov telescope development will see a great increase in both quantity and quality of γ-ray morphological data. This initiated the development of a spatiotemporal leptonic transport code ... -
Jovian electrons in the inner heliosphere: proposing a new source spectrum based on 30 years of measurements
(EDP Sciences, 2018)Context. Since the Pioneer 10 flyby of Jupiter it has become well known that electrons of Jovian origin dominate the lower MeV range of charged energetic particles in the inner heliosphere. Aims. Because the Jovian source ... -
Numerical modeling of galactic cosmic-ray proton and helium observed by AMS-02 during the solar maximum of solar cycle 24
(IOP Publishing, 2019)Galactic cosmic rays (GCRs) are affected by solar modulation while they propagate through the heliosphere. The study of the time variation of GCR spectra observed at Earth can shed light on the underlying physical ...