Results 261 to 270 of about 41,384 (308)

The Energetic Particle Detector. Energetic particle instrument suite for the Solar Orbiter mission

open access: yes, 2019
Rodriguez-Pacheco, J   +5 more
openaire   +1 more source

On energetic particles in space

open access: yesActa Physica Slovaca. Reviews and Tutorials, 2009
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
openaire   +2 more sources

Energetic Charged Particles in the Terrestrial Magnetosphere: Cluster/RAPID Results

open access: yesJournal of Geophysical Research: Space Physics, 2021
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
exaly   +2 more sources

Energetic Particle Observations

Space Science Reviews, 2006
The 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
openaire   +4 more sources

Energetic Particles in the Jovian Magnetotail

Science, 2007
When 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
openaire   +2 more sources

Energetic Particles at High Latitudes

Space Science Reviews, 1995
We 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
openaire   +1 more source

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