Automatic resonance recognition method in solar wind

Details Automatic resonance recognition method in solar wind Automatic resonance recognition method in solar wind

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ncimc...3..696t&link_type=abstract

Nuovo Cimento C, Serie 1, vol. 3C, Nov.-Dec. 1980, p. 696-710.

Computer Science

Sound

Plasma Frequencies, Plasma Resonance, Signal Reception, Solar Terrestrial Interactions, Solar Wind, Automatic Control, Magnetospheric Electron Density, Onboard Data Processing, Satellite Sounding, Spacecraft Trajectories

Scientific paper

The principal objective of the Sounder experiment aboard ISEE 1 is to study the plasma frequency along the spacecraft trajectory. This represents a considerable amount of data for the duration of the mission (three years). Thus an automatic method is necessary to recognize the plasma resonances. A resonance recognition methodology based on the Sebestyen's discrimination approach is presented. The preliminary results of this method, obtained from a set of known resonances, show a good efficiency (more than 90 percent of the known plasma resonances are recognized). This method will be used in the future to identify other resonances in the magnetosphere.

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