The real-time classification of solar-wind ions in the SWICS experiment of the ISPM mission

Details The real-time classification of solar-wind ions in the SWICS experiment of the ISPM mission The real-time classification of solar-wind ions in the SWICS experiment of the ISPM mission

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981dglr.meet.....g&link_type=abstract

Deutsche Gesellschaft für Luft- und Raumfahrt, Jahrestagung, Aachen, West Germany, May 11-14, 1981, 10 p. In German.

Computer Science

Ion Emission, Solar Spectrometers, Solar Wind, Ulysses Mission, Particle Mass, Particle Motion, Plasma Composition, Taylor Series

Scientific paper

It is the main objective of the Solar Wind Ion Composition Spectrometer (SWICS) to obtain data regarding the composition of the solar wind, taking into account mass, electrical charge, velocity, and direction of motion of the particles. The employed measurement procedures are discussed along with the classification of the ions, aspects of system optimization according to three quality criteria, the implementation of the classification procedure, the structure of table classification, and the use of the Taylor approximation. A block diagram of the classification unit is presented, giving attention to the NQ grid tables, the NM grid tables, and the bin address tables.

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