A new approach to the investigation of the large-scale structure of the solar corona based on measurements of solar-wind parameters

Details A new approach to the investigation of the large-scale structure of the solar corona based on measurements of solar-wind parameters A new approach to the investigation of the large-scale structure of the solar corona based on measurements of solar-wind parameters

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kosis..28..890y&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 28, Nov.-Dec. 1990, p. 890-902. In Russian.

Physics

2

Alpha Particles, Coronal Holes, Solar Corona, Solar Protons, Solar Wind, Current Sheets, Heliosphere, Solar Magnetic Field

Scientific paper

The structure of the solar wind is investigated on the basis of
selective measurements of proton and alpha-particle bulk parameters and
the magnetic field via the Prognoz-7 satellite. Five regions (or types
of wind streams) are identified which may be connected with the
structure of the solar corona.

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