Chemical composition of the solar wind (measurement possibilities of the plasma experiment of the HELIOS probe)

Details Chemical composition of the solar wind (measurement possibilities of the plasma experiment of the HELIOS probe) Chemical composition of the solar wind (measurement possibilities of the plasma experiment of the HELIOS probe)

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hsde.rept...41m&link_type=abstract

In Arbeitsgemeinschaft für Weltraumforsch. Helios Satellite Sci. Data Evaluation p 41-51 (SEE N75-23393 14-88)

Computer Science

Chemical Composition, Heavy Ions, Helios Project, Solar Wind, Satellite-Borne Instruments, Solar Corona, Velocity Distribution

Scientific paper

The possible objectives of heavy ion observation in the solar wind and the measurement possibilities of the Helios plasma experiment are discussed. The unintentional recording of heavy ions can be made useful for several reasons, among which the knowledge of transport phenomena between photosphere and corona. The possibility is considered of three dimensional measurement of the solar wind spectrum with the 15-channel mass spectrometer, and also the temperature of heavy ions.

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