Observation of singly ionized helium in the solar wind

Details Observation of singly ionized helium in the solar wind Observation of singly ionized helium in the solar wind

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..717y&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, Sept.-Oct. 1989, p. 717-725. In Russian.

Computer Science

Helium Ions, Ionized Gases, Prognoz Satellites, Solar Wind, Heavy Elements, Interplanetary Medium, Mass Spectroscopy, Solar Corona, Solar Temperature, Stellar Mass Ejection

Scientific paper

Prognoz-10-Intercosmos mass-spectrometer measurements of the anomalous ion composition of the solar wind on April 30, 1985 are presented. Besides highly ionized heavy-element ions formed ion the hot coronal plasma, He(+) ions were detected which can form only at temperatures significantly below coronal ones. The data suggest that the observed event is connected with coronal-mass ejection.

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