Physics
Scientific paper
Sep 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974kosis..12..716z&link_type=abstract
Kosmicheskie Issledovaniia, vol. 12, Sept.-Oct. 1974, p. 716-724. In Russian.
Physics
1
Alpha Particles, Satellite-Borne Instruments, Solar Protons, Solar Wind, Spectral Energy Distribution, Energy Spectra, Helium Ions, Hydrogen Ions, Solar Flares, Solar Flux Density
Scientific paper
The energy spectra of solar-wind H+, He++, and He+ ions were measured with an energy-mass analyzer on board a high-apogee satellite. Output signal recordings at intervals of 1.28 sec made it possible to discern rapid flux fluctuations at various energy levels for each of the ion species. It was found that the spectral flux density of alpha-particles varies appreciably in time and is substantially greater than that of the protons. The increase in the fluctuation level for alpha-particles is attributed to the influence of a helium-rich plasma from a solar flare.
Khokhlov M. Z.
Vaisberg Oleg L.
Zastenker Georgy N.
Zertsalov A. A.
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