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Emergent charge crystallization and frustration in a particle anti-spin Ice
Tierno P, Baillou R, Terkel M, Nisoli C.
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The Energetic Particle Detector. Energetic particle instrument suite for the Solar Orbiter mission
Rodriguez-Pacheco, J +5 more
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On energetic particles in space
On energetic particles in spaceParticles energized above the Earth's atmosphere provide unique informations about specific physical processes in the outer space. This is an attempt to present a short review of the knowledge of the characteristics of the cosmic energetic particles in wide energy range as observed on the ground, in the atmosphere, on ...
K. Kudela
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Energetic Charged Particles in the Terrestrial Magnetosphere: Cluster/RAPID Results
In this work, we review the results of observations by the Cluster/Research with Adaptive Particle Imaging Detectors (RAPID) energetic charged particle detector (~40 keV–~1 MeV).
E A Kronberg, P W Daly, E E Grigorenko
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Energetic Particle Observations
Space Science Reviews, 2006The characteristics of solar energetic particles (SEP) as observed in interplanetary space provide fundamental information about the origin of these particles, and the acceleration and propagation processes at the Sun and in interplanetary space. Furthermore, energetic particles provide information on the development and structure of coronal mass ...
Klecker, B. +16 more
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Energetic Particles in the Jovian Magnetotail
Science, 2007When the solar wind hits Jupiter's magnetic field, it creates a long magnetotail trailing behind the planet that channels material out of the Jupiter system. The New Horizons spacecraft traversed the length of the jovian magnetotail to >2500 jovian radii ( R J ; 1 R J
R L, McNutt +19 more
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Energetic Particles at High Latitudes
Space Science Reviews, 1995We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path λ r which is approximately constant as a function of ...
R. M�ller-Mellin, G. Wibberenz
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