Computer Science
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978clus.nasa..173g&link_type=abstract
In JPL A Close-up of the Sun p 173-190 (SEE N78-32964 23-92)
Computer Science
Energetic Particles, Ion Density (Concentration), Particle Acceleration, Solar Corona, Solar Flux Density, Solar Probes, Abundance, Energy Spectra, Kinetic Energy, Mission Planning, Solar Instruments, Solar Wind
Scientific paper
The energy spectra and composition of particles escaping from the Sun provide essential information on mechanisms responsible for their acceleration, and may also be used to characterize the regions where they are accelerated and confined and through which they propagate. The suprathermal energy range, which extends from solar wind energies (approximately 1 KeV) to about 1 MeV/nucleon, is of special interest to studies of nonthermal acceleration processes because a large fraction of particles is likely to be accelerated into this energy range. Data obtained from near earth observations of particles in the suprathermal energy range are reviewed. The necessary capabilities of an a ion composition experiment in the solar probe mission and the required ion measurements are discussed. A possible configuration of an instrument consisting of an electrostatic deflection system, modest post acceleration, and a time of flight versus energy system is described as well as its possible location on the spacecraft.
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