Large-scale structure of solar wind and its relationship with solar corona - Prognoz 7 observations

Details Large-scale structure of solar wind and its relationship with solar corona - Prognoz 7 observations Large-scale structure of solar wind and its relationship with solar corona - Prognoz 7 observations

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991p%26ss...39.1351y&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 39, Oct. 1991, p. 1351-1361.

Physics

7

Magnetic Field Configurations, Magnetohydrodynamics, Solar Corona, Solar Magnetic Field, Solar Wind, Ion Density (Concentration), Prognoz Satellites, Solar Physics, Solar Wind Velocity, Stellar Structure

Scientific paper

The structure of solar wind is studied using data on proton and alpha-particle bulk parameters and magnetic field obtained by Prognoz 7 satellite. For that purpose, the magnetic field value B, the proton temperature Tp, the relative helium abundance (n-apha/n-p), and the ratio between thermal and magnetic pressures beta = nkTp/(B-sq/8 pi) are represented as distributions on the n-Vp (solar wind ion density-proton velocity) plane. The values and behaviors of these parameters on the n-Vp plane are used to identify five regions (types of solar wind streams) which may be connected with well known solar corona structure and events.

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