2012
DOI: 10.1016/j.cpc.2012.07.005
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Comparative study of forward and backward test-kinetic simulation approaches

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Cited by 6 publications
(2 citation statements)
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“…The background magnetic field is assumed to be dipolar with equatorial strength at the Earth's surface of    with 64 points (particles with initial velocities larger than E c are excluded from the sample). To confirm that this resolution is sufficient (Voitcu et al, 2012), we limited the range in velocities to focus on the resonance region of the first subpacket, and doubled the number of gyrophase grid points. Apart from some finer features associated with the phase mixing of lower and higher density regions, there was no noticeable difference.…”
Section: Backward-in-time Test Particle Simulationmentioning
confidence: 99%
“…The background magnetic field is assumed to be dipolar with equatorial strength at the Earth's surface of    with 64 points (particles with initial velocities larger than E c are excluded from the sample). To confirm that this resolution is sufficient (Voitcu et al, 2012), we limited the range in velocities to focus on the resonance region of the first subpacket, and doubled the number of gyrophase grid points. Apart from some finer features associated with the phase mixing of lower and higher density regions, there was no noticeable difference.…”
Section: Backward-in-time Test Particle Simulationmentioning
confidence: 99%
“…Crescent-like VDFs were observed for ions in the Earth's magnetotail, close to the neutral sheet and plasma sheet boundary layer (e.g. Nakamura et al, 1991Nakamura et al, , 1992Wilber et al, 2004), as well as in the magnetosheath, close to the magnetopause (e.g. Marcucci et al, 2004).…”
Section: Introductionmentioning
confidence: 99%